The galaxy appears to be a relatively compact system. Its morphology suggests a predominantly smooth, spheroidal shape. However, there may be some evidence of disk-like or featured structures, potentially indicating ongoing or past interactions. The galaxy exhibits a concentrated central region with a gradual decrease in luminosity outwards. The color profile indicates a redder overall composition, suggestive of an older stellar population with relatively low star formation activity. Some disturbances appear to be present, possibly indicating a tidal interaction. A possible merger is also consistent with these findings.
