The galaxy presents as a relatively smooth, elliptical-like structure with no apparent spiral arms or a distinct disk component. It exhibits a centrally concentrated luminosity profile, appearing brightest towards the core region, with the brightness gradually diminishing outwards. The galaxy's color appears to be a slightly redder hue, suggesting a potentially older stellar population and/or significant dust content. There is no visual evidence of ongoing major mergers or strong tidal disturbances; however, subtle irregularities or faint extensions might be present upon closer inspection. The overall morphology is consistent with an early-type galaxy undergoing relatively low levels of star formation. The galaxy's shape is generally round.
