The galaxy presents as a relatively smooth, elliptical morphology. Its color profile is dominated by redder wavelengths, suggesting a population of older stars, with an apparent lack of significant dust lanes or ongoing star formation regions discernible in the image. The galaxy's shape is largely spheroidal, with an approximate apparent diameter of around 3 arcseconds. There is a slight indication of elongation, but its structure is primarily consistent with an early-type galaxy that is not currently undergoing any major mergers or disturbances. 
