The galaxy presents as an elliptical or lenticular structure with a smooth, diffused appearance. It has a centrally concentrated light profile, with a gradual decrease in surface brightness outward from the core. The galaxy exhibits a generally round shape. There is a slight elongation or flattening to the overall structure. The color index suggests a population of older stars, with a dominant redder hue overall, however, the bluer light may hint at some degree of star formation activity. No signs of prominent spiral arms, bars, or significant dust lanes are observed. No evidence of major mergers or tidal disturbances is apparent.
