The galaxy presents as a flattened elliptical, with a noticeable elongation along its major axis. The light distribution suggests a smooth, centrally concentrated bulge that dominates the overall luminosity. The color gradient transitions from a yellowish core to slightly bluer, more diffuse edges. There is no evidence of strong spiral arm structure or prominent dust lanes. The overall morphology indicates a relatively evolved system, potentially transitioning towards a lenticular (S0) type galaxy, exhibiting a low rate of star formation. There is a small amount of asymmetrical distortion, possibly indicating a recent or ongoing minor merger.
