The galaxy presents as a centrally concentrated object with a generally smooth morphology. The primary body of the galaxy exhibits a largely spheroidal shape, with a subtle elongation along one axis, but it appears close to round. The light distribution suggests a relatively even distribution of stars, with no significant spiral arm structures or bar features immediately apparent. The color profile indicates a dominant population of older stars, contributing to a reddish hue in the outer regions. The core region shows a slight bluer tint, which could point to pockets of younger, hotter stars, or potentially the presence of an active galactic nucleus, although further spectroscopic data would be needed to confirm. There appear to be minimal signs of ongoing or recent major mergers, though slight asymmetries might indicate minor past disturbances or interactions. Overall, the galaxy is likely an elliptical or lenticular type, consistent with a relatively quiescent star formation history.
