The galaxy presents as a predominantly smooth, elliptical morphology. It exhibits a concentration of light towards the center, suggesting a prominent galactic nucleus. The object appears to be generally round. There is minimal evidence of spiral arms or a defined disk structure in this particular observation. Color gradients are subtle, with a possible shift towards redder hues in the central region, potentially indicative of an older stellar population. The outer regions show some blue hues. There is no sign of it currently undergoing a major merging event, however there is some evidence that it may have undergone a minor disturbance in the past.
