The galaxy presents as a centrally concentrated object, appearing largely smooth in morphology. There is minimal discernible structure, suggesting a lack of spiral arms or a prominent disk. The light profile exhibits a relatively high degree of circularity, with no obvious elongation or tidal features. 

The color gradient indicates a population of older stars. The core displays a slightly yellowish hue, likely attributed to an accumulation of older, less massive stars. Fainter blue colors can be observed in a halo surrounding the yellow core.

The light is extended, though not substantially, beyond the bright core. The absence of distinct tidal tails or streams suggests no recent major mergers or strong gravitational interactions. However, a faint, asymmetric feature to the right of the core might indicate a minor disturbance. Based on color and morphology, this galaxy is likely an elliptical galaxy undergoing minimal star formation.
