The galaxy presents as an elliptical or lenticular system, exhibiting a relatively smooth, featureless morphology. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness outwards from the core. The shape is elongated, but not highly so. There is a color gradient, with the central region displaying a bluer hue transitioning to a redder color in the outer regions. This color variation could indicate differing stellar populations, with younger, bluer stars concentrated in the nucleus and older, redder stars dominating the outer halo. There is no clear evidence of spiral arms, dust lanes, or recent merger activity. A possible slight disturbance is indicated by the asymmetry in the outer halo region. Overall, the galaxy appears to be a relatively evolved system, and we can infer its star formation rate is rather low.
