The galaxy presents an elliptical morphology, with a smooth and largely featureless appearance. The core region exhibits a higher surface brightness and a slightly redder hue, indicative of an older stellar population. Moving outward from the center, the galaxy transitions to a slightly bluer color, suggesting the presence of younger stars in the outer regions, although to a minimal amount. The overall shape is moderately elliptical, with a discernible elongation along one axis. There is no evidence of prominent spiral arms, bars, or significant dust lanes. The galaxy does not show signs of major mergers or tidal disturbances. It appears as a relatively isolated system, gravitationally undisturbed.
