The galaxy presents as a somewhat diffuse, flattened elliptical morphology, although not extremely elongated. Its central bulge is prominent, exhibiting a concentrated, yellowish-white hue, suggesting a population of older stars. Moving outward from the center, the galactic disk is faintly visible, showing hints of spiral structure that are not well-defined. The color in the outer regions shifts towards a bluer tint, possibly indicating the presence of younger, hotter stars and some ongoing star formation activity. Overall the galaxy appears fairly smooth, however, there is a slight suggestion of a minor disturbance or interaction, visible as an asymmetry in the outer disk. The apparent size of the galaxy suggests it is a relatively large and massive system.
