The galaxy appears to be a relatively smooth, centrally concentrated object. It displays a roughly elliptical morphology, appearing somewhat rounded, with an intermediate ellipticity. A faint, diffuse disk or extended structure is suggested, though not clearly defined. The galaxy presents a color gradient, with a brighter, yellower core transitioning to a redder hue in the outer regions. There are some faint, irregular features, possibly indicative of minor disturbances or ongoing interactions. Overall, the galaxy's appearance suggests a system with a relatively quiescent star formation rate, and a significant fraction of evolved stellar populations, with a stellar mass in the range of 10^10 to 10^11 solar masses.
