The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity outwards. The galaxy's color profile suggests an older stellar population, with a yellow/red hue. There's minimal evidence of spiral arm structures or significant dust lanes. The overall morphology indicates it is a relatively relaxed galaxy. The light distribution is largely symmetrical, with no major disturbances or signs of ongoing mergers apparent in the immediate vicinity of the core. The galaxy appears to be somewhat compact.
