The galaxy exhibits a generally smooth morphology, though with some indications of internal structure suggesting a possible disk-like component. Its overall shape appears to be somewhere between round and elongated, with a tendency toward the elongated side. There is no obvious evidence of a major ongoing merger, although subtle distortions may hint at past or minor interactions.

The color profile suggests the presence of both older stellar populations and ongoing or recent star formation activity. The galaxy's substantial estimated mass indicates it is a relatively large system. Based on the data and the image, the galaxy appears to have a suppressed specific star formation rate, suggesting it is transitioning towards a more quiescent state. The galaxy is relatively far away, and while we cannot see major details of it, we can still get a sense of its overall characteristics and history.