The galaxy presents as a relatively smooth, centrally concentrated structure. The light profile appears to be largely spheroidal with a bright, slightly yellowish core that fades smoothly into the surrounding halo. There is a noticeable lack of distinct spiral arm features or significant dust lanes. The galaxy appears highly rounded in shape with no evidence of major distortions or ongoing mergers. Subtle color variations suggest some radial stratification in the stellar populations with the central region appearing relatively older and redder compared to the outer regions. Overall, the galaxy appears to be an elliptical galaxy, characterized by a generally smooth appearance without prominent features.
