The galaxy exhibits a morphology consistent with an elliptical galaxy or a lenticular galaxy seen nearly face-on. The light distribution appears centrally concentrated, displaying a smooth, diffuse profile. There is a bright, yellowish core which gradually fades into an outer halo. The isophotes appear generally elliptical, with the major axis and minor axis of the galaxy being roughly similar in length. No distinct spiral arm structures or prominent dust lanes are apparent in this image, suggesting a lack of significant recent star formation activity. A slight elongation or tidal disturbance might be present at the bottom of the galaxy, potentially indicating a past or ongoing interaction with another galaxy, but this is not definitive. The overall color suggests an older stellar population, with light dominated by redder wavelengths.
