The galaxy exhibits a smooth, elliptical morphology. It appears relatively undisturbed, showing no strong signs of recent or ongoing major mergers. A central bulge is prominent, exhibiting a concentrated luminosity gradient. The isophotes appear mostly concentric. The galaxy displays a yellowish-red hue, suggestive of an older stellar population with diminished ongoing star formation. There is faint evidence of a disk-like structure, viewed nearly edge-on. There appears to be minor presence of a spiral arm. The overall color profile indicates a higher concentration of older stars.
