The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and featureless morphology. There is a slight elongation observed, although the overall shape is closer to round than cigar-shaped. The galaxy presents a centrally concentrated luminosity profile, with the light intensity gradually decreasing towards the outer regions. There is no apparent evidence of spiral arms or a prominent disk structure. Based on its red color, the galaxy likely consists of an older stellar population, potentially indicating a relatively low rate of ongoing star formation. There appears to be no significant sign of any major ongoing merger activity, although there may be some minor disturbances in the outer regions. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
