The galaxy presents as a relatively smooth, elliptical-like structure, though not perfectly spherical. The primary body exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer edges. Coloration suggests an older stellar population, with a yellowish-red hue dominating. There appears to be some level of gravitational interaction occurring with a smaller, irregular structure nearby on the edge of the primary galaxy, which may indicate tidal disturbances. This second structure appears to be bluer in color, so may show recent star formation. Overall, the galaxy is neither highly disturbed nor perfectly symmetric, exhibiting subtle signs of potential past or ongoing interactions.
