The galaxy presents as a relatively smooth, elliptical object. It exhibits a centrally concentrated luminosity profile, indicating a high stellar density in the core region. The galaxy appears largely featureless, lacking prominent spiral arms or distinct dust lanes. The central region displays a slightly redder hue compared to the outer regions, which transition towards a bluer color profile, suggesting a difference in stellar populations with the core likely dominated by older, redder stars, while the outer regions may contain a population of younger, bluer stars. The overall shape appears moderately elliptical, with a noticeable elongation along one axis. No signs of ongoing major mergers or significant tidal disturbances are readily apparent. The galaxy exhibits a gradual decline in surface brightness from the core to the outskirts, with no sharp edges or truncations observed.
