The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light profile appears to be centrally concentrated, gradually fading towards the outer edges. The color is generally consistent, with a slight bluing trend towards the outer regions. No strong dust lanes or spiral arm features are discernible. There is no obvious sign of a major merger event, although a slight asymmetry could indicate a minor interaction. Overall, the galaxy exhibits characteristics of a relatively evolved system.
