The galaxy presents as a relatively smooth, centrally concentrated elliptical morphology. The central region exhibits a bright, yellowish hue suggestive of an older stellar population. Progressing outward from the core, the color gradually transitions to a bluer shade, indicative of younger stars or potentially ongoing, but suppressed, star formation activity. The overall structure appears largely undisturbed, with no immediately obvious signs of major mergers or significant tidal interactions. There are some subtle irregularities in the outer regions which could indicate a minor disturbance. The galaxy exhibits an approximately elliptical shape with a ratio of major to minor axis close to 1.0.
