This galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, surrounded by a more diffuse halo. The color profile suggests a dominant population of older stars, contributing to the yellowish hue observed. There is some indication of a slight, subtle disk present, but the galaxy is largely spheroidal. The galaxy appears to be largely undisturbed, showing no strong signs of recent merger activity or tidal features. Overall, this galaxy appears as a relatively evolved system, with a minimal star formation rate.
