The galaxy presents as a somewhat smooth, centrally concentrated object with a subtle disk-like structure. The central bulge appears prominent, exhibiting a yellowish hue, indicative of an older stellar population. Fainter, bluer regions are observed within the disk component, suggesting some ongoing star formation, although at a relatively low rate. The overall shape is generally round, with only minor disturbances visible in its morphology. There is some indication of possible tidal interactions or minor merging events.
