The galaxy presents a generally smooth appearance with a roughly elliptical morphology. It appears to have a core of concentrated light with lower surface brightness extending outwards. There is a slight color gradient that appears to become redder towards the outskirts. The galaxy appears to be a relatively isolated system with some subtle disturbances visible, possibly indicative of a past or ongoing interaction with a smaller companion. Further spectral analysis would be useful to determine the age and metallicity of the stellar populations within the galaxy and constrain its star formation history.
