This galaxy exhibits a somewhat irregular morphology. The central region appears relatively smooth and concentrated, suggesting a possible bulge component. Surrounding this bulge, fainter, diffuse emission is visible. This fainter emission is not uniform, showing hints of a possible disk-like structure or tidal disturbances. There is a slight elongation to the galaxy's overall shape, giving it an oval appearance. Color gradients are visible, with the central region appearing whiter and bluer, while the outer regions appear more reddish in comparison. The redness in the outer regions may indicate an older stellar population, whereas the bluer center possibly harbors younger stars and ongoing star formation. There seems to be evidence of a potential interaction, given the disturbed or irregular features extending from the main body of the galaxy. However, these features are subtle and could also be due to internal dynamics. Overall, this galaxy presents a complex morphology, with features suggesting both a smooth bulge and a potentially disturbed disk.
