The galaxy appears to be a relatively smooth, elliptical-type galaxy. The central region exhibits a high concentration of light, appearing bright and yellowish in color. Moving outwards from the center, the light intensity decreases gradually, forming a more diffuse halo. There is a subtle color gradient, shifting slightly towards redder hues in the outer regions. The overall shape is generally round, with no obvious signs of strong tidal distortions or major mergers. There is a possible faint feature or disturbance in the lower central part of the galaxy, that could potentially indicate a minor interaction. Based on the color profile, we can infer there may be older stellar populations dominating the galaxy's composition, implying a relatively low rate of star formation.
