The galaxy presents a generally smooth morphology with a slightly elongated profile, appearing more in between round and cigar shaped. It is a centrally concentrated system, exhibiting a core region that graduates into a less dense, more diffuse outer envelope. The core displays a reddish-orange hue, possibly indicating an older stellar population with minimal ongoing star formation. Moving outward, the color transitions to a slightly bluer tint, hinting at the presence of some younger stars. No prominent spiral arms or distinct features like dust lanes are discernible, suggesting the galaxy is likely an elliptical type or a lenticular galaxy viewed at a low inclination. There is no apparent evidence of any major mergers or strong tidal disturbances and only slight possibilities of minor disturbances.
