The galaxy appears as a singular, relatively smooth object with a roughly round morphology. Its light profile suggests a concentration towards the center, characteristic of an elliptical galaxy or a spiral galaxy viewed face-on with a dominant bulge.

The galaxy's color appears yellowish-orange, suggestive of an older stellar population. The lack of distinct blue regions indicates a low rate of ongoing star formation.

There is a slight asymmetry in its overall shape, possibly indicating a minor gravitational interaction or internal disturbance, but this could also be due to image artifacts. No prominent spiral arms, bars, or tidal tails are readily discernible. The galaxy does not appear to be undergoing a major merger event based on its morphology.
