The galaxy presents as a generally smooth, elliptical-like structure. It appears to be elongated, with the major axis significantly longer than the minor axis. The light distribution indicates a concentrated central bulge, possibly harboring an active galactic nucleus. The color profile is generally redder in the central regions, suggesting an older stellar population. There is a subtle gradient toward bluer colors in the outer regions, hinting at ongoing or recent star formation, although not particularly pronounced. No obvious spiral arm structures or dust lanes are visible. A faint, diffuse halo may be present, extending beyond the main body of the galaxy. There is no obvious evidence of a major merger event or significant tidal disturbances. A minor companion galaxy may be in the vicinity, but its relation to the galaxy is unclear.
