The galaxy appears to be an elliptical, exhibiting a generally smooth morphology with little discernible internal structure. It has a concentrated central bulge that emits strongly in the g, r, and z bands. The galaxy has a slightly elongated, though largely rounded shape. There is no obvious evidence of a prominent disk or spiral arms. Minimal tidal features or distortions suggest it is not currently undergoing a major merger, though some minor disturbances cannot be ruled out at this resolution. Based on the color profile, this galaxy likely contains a population of relatively older stars, potentially implying a low ongoing rate of star formation.
