The galaxy presents as a largely featureless elliptical morphology. The light profile is centrally concentrated, with a gradual decrease in surface brightness extending outwards. The core region exhibits a yellow hue, suggesting a population of older, evolved stars. Fainter, diffuse light surrounding the core is slightly more reddish, potentially indicating the presence of a small amount of dust or a redder stellar population within the outer regions. No prominent spiral arms or bar structures are visible. The overall shape is largely circular, exhibiting very little ellipticity, indicating a classification tending more towards E0 than a highly elongated elliptical galaxy. There is no visually detectable ongoing major merger event, however, a minor disturbance is possible, given the slight irregularities in the faint outer halo. The galaxy appears relatively isolated.
