The galaxy presents as a centrally concentrated, smooth object with a predominantly elliptical morphology. The core exhibits a strong, reddish-yellow hue, indicative of an older stellar population. The luminosity appears to diminish gradually from the center outwards, with a broader, more diffuse halo extending into the surrounding space. 

A faint blue arm or tidal tail is present on one side of the galaxy, suggesting a possible interaction or past merger event. This region displays bluer colors, suggestive of ongoing or recent star formation. There appears to be little dust in the main body. Overall, the galaxy exhibits characteristics of a relatively massive system, with a substantial, quiescent stellar population and evidence of past or ongoing interactions.
