The galaxy presents as a smooth, relatively featureless object. Its overall shape appears to be elliptical, leaning toward a slightly oblate spheroid, but not quite a cigar shape. The core exhibits a concentrated brightness, suggesting a high stellar density. The central region displays a yellowish hue, potentially indicative of an older stellar population. Moving outwards from the core, the color transitions subtly to a greenish tint, hinting at the presence of some younger stars and perhaps regions of ongoing, albeit subdued, star formation. There is no visible evidence of spiral arms or a prominent disk structure. The galaxy seems relatively isolated, with no apparent signs of tidal interactions or ongoing mergers.
