The galaxy appears as a luminous, centrally concentrated object. It presents a somewhat elliptical morphology, with a major axis that seems to be slightly more extended than its minor axis. The light distribution is smooth, suggesting a relatively uniform stellar population. There is a subtle color gradient, shifting from a bluer hue towards the center to slightly redder colors in the outer regions. This could indicate older stars residing in the outer parts of the galaxy. There might be some minor irregularities along its edges, possibly hinting at gravitational interactions or recent accretion events.
