The galaxy presents as a relatively smooth, elliptical-like structure. Its light distribution is centrally concentrated, with a bright, diffuse core. The galaxy appears mostly featureless, lacking prominent spiral arms or significant dust lanes. A slight elongation is observed, deviating from a perfect circular shape. The color profile suggests an older stellar population, with a yellow/red hue dominating the central region, with some hints of younger, bluer stars present. There does not appear to be any evidence of a major ongoing merger or significant tidal disruption. There may be hints of a very minor disturbance near the lower region of the disk, but this could also be image noise. Overall, the galaxy appears to be a relatively quiescent system.
