The galaxy presents a somewhat elliptical morphology, appearing neither perfectly spherical nor highly elongated. The light distribution is relatively smooth, suggesting a lack of prominent spiral arms or significant clumpy star-forming regions. There is a subtle central concentration of light, potentially indicating a galactic nucleus or bulge. Faint extensions or tidal features are not readily apparent, implying the absence of recent major merger events. The color appears to be moderately red, which could indicate an older stellar population or significant dust obscuration. Overall, the galaxy appears to be a relatively quiescent system with a smooth, centrally concentrated light profile, and a red color.
