The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits an elliptical morphology, lacking prominent spiral arms or a distinct disk structure. The central bulge region is bright, possibly indicating a high stellar density or the presence of an active galactic nucleus. The color gradient suggests a population of older stars, with a general redder hue overall. There's a slight elongation in the galaxy's shape, tending towards a cigar-like appearance. No significant signs of major mergers or tidal disturbances are apparent, and instead, it is relatively undisturbed.
