The galaxy appears to be an elliptical type, characterized by a smooth, symmetrical light distribution. The core region exhibits a concentrated, bright glow, fading gradually outward into a less luminous halo. The overall color profile suggests an older stellar population, leaning towards redder wavelengths. There is a small, distinct knot of reddish light located off-center. While the galaxy seems largely undisturbed, the light knot hints at a possible minor interaction or internal feature. Based on the light profile and color, star formation activity is likely low or negligible.
