The galaxy presents as a single, relatively concentrated object with a smooth overall morphology. It exhibits a slightly elongated shape, deviating marginally from perfect circularity. The central region appears bright and concentrated, suggesting a high density of stars or an active galactic nucleus. Fainter, diffuse light extends outwards from the core, forming a faint halo or envelope. The color profile is subtly varied; the central bulge shows a yellowish-white hue, possibly indicative of an older stellar population. The outer regions display a bluer tint, hinting at the presence of younger, hotter stars or ongoing star formation. There is some evidence of minor disturbances in the galaxy's structure, perhaps a slight asymmetry or a hint of tidal features, potentially indicating past or ongoing interactions with another galaxy. These disturbances are subtle, however, and do not disrupt the galaxy's overall smooth appearance. The object appears to be a galaxy with a centrally concentrated bulge and a relatively quiescent disk.
