The galaxy exhibits a generally smooth morphology, lacking prominent spiral arms or a distinct disk structure. It presents a relatively rounded appearance, with a concentrated central bulge dominating the overall luminosity. The color profile suggests a population of older stars, potentially indicating a lower rate of ongoing star formation. While there are no obvious signs of tidal disturbances or interactions, subtle asymmetries in the outer regions could be indicative of minor past mergers. The galaxy's size appears relatively compact. Overall, the galaxy appears to be a quiescent system, likely an elliptical galaxy at moderate redshift.
