The galaxy presents as a well-defined elliptical form, exhibiting high level of smoothness in its light distribution.  There is no apparent spiral structure or prominent disk. The galaxy displays a centrally concentrated luminosity profile, with a gradual decrease in brightness towards the outer regions. There may be some evidence of minor distortions or tidal features, but it remains largely undisturbed. The object appears to be a relatively compact galaxy, with a moderate spatial extent on the sky. Its color suggests a population of older stars, given its reddish tint. There are no discernible features indicative of active star formation regions within the observed optical wavelengths.
