The galaxy presents as a relatively smooth, centralized structure. The light profile appears concentrated towards the core with a gradual decrease in intensity moving outward, suggesting an elliptical morphology or a spiral galaxy viewed face-on with a prominent bulge. The overall color is yellowish-white, indicating a stellar population dominated by older stars. There is a notable absence of distinct spiral arms or prominent dust lanes. A subtle extension or halo is visible around the main body, gradually fading into the background. There is no evidence of any major disturbances or ongoing mergers, suggesting a relatively settled and evolved system.
