The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. Its core presents a bright, somewhat compact appearance. The color profile suggests a potential mix of stellar populations, with a slightly redder hue towards the center possibly indicating older stars, while the outer regions show a hint of bluer light, hinting at the presence of younger, hotter stars. No distinct spiral arms or prominent dust lanes are discernible. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. Overall, the galaxy appears as a relatively undisturbed system, consistent with an early-type galaxy in a relatively quiescent state.
