The galaxy presents a generally smooth, elliptical morphology. The light distribution appears centrally concentrated, with a bright core that diminishes gradually towards the outer regions. There is a subtle color gradient across the galaxy, transitioning from a yellowish hue in the central bulge to a slightly bluer tint in the outer regions. The galaxy exhibits a rounded shape, lacking any significant signs of spiral arms or a prominent disk structure. There is no readily apparent evidence of ongoing major mergers or strong tidal interactions with other galaxies. The overall impression is of a relatively quiescent system dominated by an older stellar population, though some residual star formation in the outer regions cannot be ruled out.
