The galaxy presents as a dominant, centrally concentrated structure with an elliptical morphology. The core exhibits a bright, diffuse glow, suggesting a significant population of older stars and a relatively low rate of ongoing star formation. The galaxy's overall color appears redder, consistent with an evolved stellar population and potential dust obscuration.

There is a minor asymmetry present, with a slight extension or disturbance visible on one side of the main body. This may indicate a previous or ongoing interaction with a smaller companion galaxy or a tidal feature resulting from past interactions. There is a second object that appears to be in close proximity to the main galaxy, but it's unclear whether it's a physically associated satellite galaxy or a foreground object. This secondary object is smaller, and much bluer.