The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated luminosity profile. It presents a somewhat elongated, but not strongly cigar-shaped, morphology. There is no obvious disk structure or spiral arms, instead a diffuse halo of light extends outward, fading into the background. The color index appears to be relatively uniform across the galaxy, with a subtle redder hue concentrated in the center. The galaxy is compact, not showing signs of major mergers or tidal disturbances in its immediate surroundings. However, there appears to be an irregular distribution of luminosity within the halo, suggesting possible minor interactions or past mergers.
