The galaxy presents as a centrally concentrated object, elliptical in appearance with a smooth, diffuse light distribution. The central region exhibits a bright, yellow-white core, indicative of an older stellar population or potentially an active galactic nucleus, although no distinct point source is discernible. The outer regions fade gradually into the background sky, displaying a slightly redder hue compared to the central core. There is a noticeable elongation, classifying it as not perfectly spherical. No prominent spiral arms, dust lanes, or other distinct features are immediately apparent in this image, suggesting a lack of significant ongoing star formation in the outer regions. There is no visible evidence of major mergers or significant tidal disturbances.
