The galaxy presents as a disc galaxy with a moderately bright, concentrated central bulge. The bulge exhibits a bluish-white hue, possibly indicating the presence of a younger stellar population and/or active star formation. Surrounding the central bulge, there appears to be a somewhat fainter, broader disc. The disk shows evidence of a relatively uniform color distribution. The shape is fairly well-defined, with a smooth outer edge. There is some hint of a slight disturbance or asymmetry in the disc structure, possibly indicative of a minor interaction. The presence of a ring or arm-like feature could be due to tidal forces or internal dynamical processes. Overall, the galaxy appears to be a relatively normal disc galaxy with moderate signs of recent or ongoing activity.
