The galaxy presents a smooth, elongated morphology, suggestive of an elliptical or lenticular type. The light distribution appears relatively uniform, with a central concentration of older stars indicated by the yellowish hue in the core. Towards the outer regions, a faint blue tinge suggests the presence of younger stellar populations, possibly indicating ongoing or recent star formation, though limited. There is no distinct spiral arm structure, though a slight disk-like component cannot be ruled out. No signs of major mergers or significant tidal disturbances are apparent in this image. The overall structure is indicative of a relatively undisturbed, evolved galaxy.
