The galaxy presents as a centrally concentrated, smooth object with a radial color gradient. The core appears yellowish-white, transitioning to a slightly redder hue in the outer regions. No distinct spiral arms or bar structures are apparent. The overall morphology suggests an elliptical galaxy or potentially a lenticular galaxy viewed at a high inclination, where disk features are not easily discernible. There are slight distortions in the outer edges of the galaxy, suggesting potential minor gravitational interactions with nearby objects, which could have slightly disrupted the galaxy's structure. The observed color profile indicates a stellar population dominated by older, redder stars, particularly in the outer regions, hinting at a cessation of significant recent star formation activity.
