The galaxy appears to be a single, moderately sized object with a smooth light profile, lacking the distinct features of a spiral or barred galaxy. The galaxy's overall shape is somewhat elliptical, leaning towards an intermediate ellipticity with only slight elongation. The light is concentrated towards the center, with a gradual decrease in intensity towards the edges. The color gradient ranges from yellowish-white in the central region, shifting towards a slightly redder hue in the outer regions. This color difference could indicate an older stellar population in the outskirts compared to the core. The galaxy is not obviously isolated, with hints of distortions or irregular shapes in the outer edges possibly indicating gravitational interactions or recent merger events.
