The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright yellowish-white hue, suggesting a population of older stars and potentially a supermassive black hole actively accreting matter, though no distinct active galactic nucleus is readily apparent in this image. Extending outward from the core, the galaxy's color shifts to a more diffuse blueish-white, implying the presence of some younger, hotter stars, although star formation appears subdued overall. The galaxy's overall shape is elongated, appearing more cigar-shaped than circular, possibly indicating it is undergoing a mild tidal interaction or is simply shaped in that manner. There are no obvious signs of major mergers or significant disturbances in its structure. The outer regions fade gradually into the background sky, lacking any sharp boundaries or distinct spiral arm structures.
