The galaxy presents an elliptical morphology, appearing largely smooth with a concentrated central region. Its color profile suggests a dominance of older stellar populations, emitting primarily in the redder wavelengths. This is likely an early-type galaxy, possibly an elliptical or lenticular. There appears to be a mild disturbance, with a slight asymmetry visible in the galaxy's overall shape, possibly indicating a minor past merger or tidal interaction with a smaller companion. Star formation appears to be relatively quiescent.