This galaxy presents a relatively smooth, round appearance. The light profile suggests a concentrated central bulge that transitions into a more diffuse, extended halo. The dominant color is yellowish-white, possibly indicative of an older stellar population within the bulge, although some blue light is present across the face of the galaxy, indicating ongoing star formation. No distinct spiral arm structure or bar is evident. A slight asymmetry is visible, with a subtle extension of the halo on one side, although this does not seem to indicate a major merger or tidal disturbance. Overall, it appears to be a relatively massive galaxy with a mixed stellar population.
