The galaxy exhibits a morphology suggesting a smooth, elliptical form, with a significant fraction of its light concentrated towards the center, creating a bright, yellowish core. It is generally round, with a slight elongation. There appears to be a faint plume or tidal tail extending from one side of the galaxy. This could be indicative of past or ongoing interaction with another galaxy, although the main body of the galaxy itself appears relatively undisturbed. Star formation appears to be limited or absent, indicated by the lack of prominent blue regions typically associated with young, hot stars. The color profile, dominated by redder wavelengths, supports this, suggesting a population of older stars.
