The galaxy presents as a relatively smooth, elliptical-like object. The light distribution is highly concentrated towards the center, with a gradual decrease in surface brightness outwards. The central region appears more yellow/white, possibly indicating an older stellar population, whereas the outer regions look somewhat redder. The object exhibits high degree of roundness, with no obvious spiral arm structures or prominent disk features. There is a faint suggestion of a minor disturbance in the galaxy's structure, but no clear signs of ongoing major mergers or tidal interactions are visible. The galaxy appears to be relatively massive, with a low star formation rate.