The galaxy presents a generally elliptical morphology, exhibiting a centrally concentrated luminosity profile that decreases gradually toward the outer regions. The core appears bright and slightly yellowish. The radial color gradient suggests a possible variation in stellar population or dust content, potentially indicating ongoing or recent star formation activity, though at a low rate. The ellipticity is low and the galaxy is not highly elongated. There is no clear evidence of spiral arms or other distinct features, but there is a slight unevenness in the isophotes toward the outer regions of the galaxy. The galaxy appears relatively undisturbed, showing no signs of recent major mergers or tidal interactions.
