The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. It has a generally elliptical shape, displaying a slight elongation but is mostly rounded. The core region is bright and appears to be composed of older stellar populations. The galaxy lacks any discernable spiral arm structure or prominent dust lanes, suggesting it is a relatively evolved system with a low rate of current star formation. The color profile suggests a redder overall population of stars, consistent with an older, less active galaxy that is not currently undergoing any major merging events. The galaxy seems relatively undisturbed, with no significant tidal features or signs of recent interactions with other galaxies.
