The galaxy presents as a well-defined elliptical or lenticular structure, exhibiting a smooth, centrally concentrated morphology. A bright central bulge is apparent, suggesting a high density of stars in the core region. The overall shape is elongated, with an approximate axis ratio of 0.5. There is no discernible spiral arm structure, nor is there any indication of recent merger activity or tidal features in this image. The galaxy's light profile appears to be consistent with a de Vaucouleurs profile, indicating a likely early-type classification. Color gradients suggest older stellar populations dominate.
