The galaxy presents an elliptical morphology, appearing somewhat elongated rather than perfectly spherical. Its light distribution suggests a relatively smooth profile, indicative of an older stellar population with fewer prominent features such as spiral arms or active star-forming regions. A slight asymmetry is observed in the galaxy’s shape, possibly suggesting minor tidal interactions or past merger events.

The color gradient indicates a more pronounced red color, implying a population dominated by older, redder stars and a dearth of young, blue stars. The galaxy seems to have a modest estimated size. It appears to be a relatively massive system, but with low star formation activity.
