The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless morphology. It exhibits a generally round shape, with a slight elongation but lacking any discernible spiral arms or a well-defined disk structure. The light distribution is centrally concentrated, with a gradual decrease in brightness towards the outer regions. Color gradients are subtle, with a yellowish-orange hue dominating the core region, potentially indicative of an older stellar population. There is no apparent evidence of significant dust lanes or recent star formation activity. The overall appearance suggests a relatively quiescent galaxy that is not currently undergoing any major merging events or significant internal disturbances.
