The galaxy presents as a relatively compact object. Its morphology is predominantly smooth and elliptical in appearance, with a high degree of central concentration of light. There is little evidence of spiral arms or a well-defined disk structure; instead, the light distribution appears diffuse and spheroidal. The core of the galaxy displays a bright, bluish-white hue, indicative of a population of relatively young, hot stars or potentially, a contribution from an active galactic nucleus. Moving outwards from the core, the light gradually transitions to a more yellowish-red color, which could suggest an older stellar population in the outer regions. There appears to be no ongoing major merging activity, although there might be minor disturbances in the galaxy's overall structure. The lack of any strong tidal tails further supports the lack of interaction with any nearby galaxies. The overall shape appears close to round, with only a small deviation towards a cigar shape.
