The galaxy presents as a relatively smooth, elliptical morphology. There is a concentrated central bulge exhibiting a yellowish hue, indicative of an older stellar population. The surrounding halo appears more diffuse with a slightly bluer tint, potentially suggesting a younger stellar population and some ongoing star formation. The overall shape is predominantly round, with only a slight deviation towards an elongated form. There is no visible evidence of significant tidal disturbances or ongoing merger activity. It's likely a massive galaxy with moderate levels of star formation relative to its stellar mass.
