The galaxy presents a generally smooth morphology, with little evidence of distinct spiral arms or a prominent bar structure. Its overall shape appears to be mostly round. The light distribution suggests it could be classified as an elliptical galaxy, or potentially a lenticular galaxy viewed at an angle that obscures any disk-like features.

The color index indicates a population of older stars, suggesting a relatively low star formation rate. There is faint indication of blue light, which suggests a small but not insignificant amount of recent star formation activity. It does not appear to be actively undergoing a major merging event or exhibiting significant tidal disturbances.
