The galaxy presents as a relatively compact, elliptical-like structure with a smooth, concentrated luminosity profile. The central region exhibits a bright, yellowish-white core, indicative of an older stellar population likely dominating the light emission. Moving outward from the core, the color transitions to a redder hue, which could suggest the presence of a slightly cooler population. There is no apparent spiral structure or dust lanes visible in the image. The galaxy's morphology is largely undisturbed, showing no signs of major mergers or tidal interactions, though there could be minor disturbances. Overall, the galaxy appears to be a relatively quiescent system.
