This galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. The light distribution suggests a dominant bulge component, with a gradual decline in intensity moving outward from the core. There is a slight elongation present, giving it an intermediate shape between round and cigar-shaped. The galaxy exhibits a yellow-red hue, indicative of an older stellar population and minimal ongoing star formation. There is no obvious spiral structure, or significant dust lanes visible. No major disturbances or signs of an active merger are apparent, although there is a minor, smaller galaxy nearby that could potentially interact with it in the future. Overall, the galaxy appears to be a quiescent system, likely a massive elliptical galaxy that has largely exhausted its gas supply.
