The galaxy presents a generally smooth and elliptical morphology, suggesting a classification as an elliptical galaxy. Its color profile leans toward the redder end of the spectrum, indicative of an older stellar population dominated by evolved stars. The galaxy exhibits a concentrated central bulge that fades gradually outward, with no prominent spiral arms or significant dust lanes visible in this image. There is no visual evidence of ongoing major mergers or tidal disturbances, though there is a slight asymmetry present in the outer halo. The overall impression is that of a relatively quiescent, massive galaxy with a diminished rate of star formation.
