The galaxy presents a generally smooth, elliptical morphology. Its light profile appears concentrated towards the center, with a diffuse halo extending outwards. The galaxy exhibits a noticeable elongation, suggesting it may be classified as an elliptical galaxy of type E3-E5 on the Hubble sequence. The core region exhibits a yellowish hue, which could indicate an older stellar population. A slight reddish region is observable on one side of the galaxy, potentially indicating a region of on-going star formation or dust obscuration. There is no distinct spiral arm structure or bar feature apparent in this image. The smooth appearance suggests the galaxy is relatively undisturbed, with no major signs of recent mergers or tidal interactions, though there may be a minor interaction. Overall, the galaxy appears to be a relatively massive, evolved system.
