The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge region that appears slightly elongated. The color gradient transitions from a warm, possibly older stellar population in the core, indicated by the redder hue, to a bluer, potentially younger stellar population in the outer regions of the galaxy. There are slight irregularities or subtle features suggesting minor tidal interactions with other galaxies, but it is mostly undisturbed. There is evidence of star formation within the galaxy, with moderate activity indicated. The overall structure suggests an evolving system, gradually transforming into a more quiescent state.
