The galaxy presents a centrally concentrated light profile, appearing largely smooth and featureless at this resolution. Its overall color is yellowish-orange, suggesting a dominant population of older stars. There is a subtle greenish hue immediately surrounding the central region, which could indicate ongoing, but not prominent, star formation activity. The shape is generally elliptical, with a slight elongation. There is no discernible evidence of spiral arms, bars, or strong tidal disturbances, suggesting it is unlikely to be undergoing a major merger, although there may be a minor disturbance.
