The galaxy presents an overall elliptical morphology, with a smooth, concentrated central bulge. The light profile suggests a gradual decrease in luminosity from the core outwards. A faint, diffuse disk component may be present, but is difficult to distinguish due to its low surface brightness and orientation. There is little to no evidence of spiral arm structure.

The galaxy exhibits a yellow-white color, indicative of an older stellar population and potentially a lower rate of on-going star formation. The galaxy's structure appears relatively undisturbed, with no major signs of tidal interactions or recent merger events. Subtle irregularities in the outer regions could indicate minor gravitational disturbances or past interactions.
