This galaxy appears to be a relatively bright, intermediate-sized object. Its morphology is somewhat ambiguous, exhibiting characteristics of both elliptical and spiral galaxies. The central region presents a smooth, concentrated bulge, which is bright and yellowish-white in color. This suggests a population of older stars.

The overall shape is elongated, approaching a cigar shape, with an apparent disk component. However, the disk is not clearly defined by prominent spiral arms or dust lanes. Instead, there are subtle hints of a flatter structure extending outwards from the central bulge. The color of the outer regions is slightly bluer than the center, suggesting the presence of younger, hotter stars.

There is no strong evidence of a recent major merger or tidal disturbance. However, there may be minor irregularities in the outer regions, potentially indicating minor interactions or accretion events. The galaxy does not show obvious signs of active star formation across its entirety, but the bluer regions suggest some ongoing activity. The galaxy appears to be relatively isolated in its immediate environment.
