The galaxy presents a generally smooth and elliptical morphology, with a concentrated central bulge exhibiting a yellowish hue, likely indicative of an older stellar population. The outer regions display a fainter, diffuse structure. There is a slight asymmetry, with a subtle extension or potential tidal feature visible on one side, possibly suggesting a minor gravitational interaction. The overall color gradient suggests ongoing or recent star formation activity, predominantly in the outer regions of the galaxy. The galaxy appears relatively isolated, lacking a clear companion within immediate proximity, although subtle disturbances could point to past or ongoing interactions.
