The galaxy presents a primarily smooth morphology, exhibiting a central bulge with a relatively high degree of symmetry. The overall shape tends toward an elliptical form, showing a lack of significant spiral arm structures or a well-defined disk. Color gradients are subtle, with the central region displaying a slightly yellower hue, potentially indicating a population of older stars. Fainter, bluer regions extending away from the central bulge are also present, suggestive of some ongoing star formation. There are some minor signs of disturbance, with some asymmetry, but does not appear to be involved in any major merging activity.