The galaxy presents as a somewhat diffuse, elliptical object. Its light profile appears relatively smooth, with a slight concentration towards the center. While not perfectly spherical, it lacks any distinct spiral arm structures or obvious bar features, implying a generally spheroidal morphology. There is a hint of a flattened disk-like component, but it's not well-defined.

The galaxy exhibits a yellowish-red hue, suggesting a stellar population dominated by older, redder stars. Some subtle color variations might be present, with bluer regions potentially indicating younger star formation areas. However, these features are subdued and indicate a low overall rate of star formation.

The lack of strong dust lanes or prominent HII regions supports the idea that the galaxy is relatively quiescent in terms of current star formation activity. There appear to be no signs of strong tidal disturbances, such as extended tails or asymmetries, though the possibility of a past minor interaction cannot be ruled out due to the somewhat irregular outer isophotes.
