The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. The nucleus is a bright, yellowish hue, suggestive of an older stellar population. The outer regions display a gradual fading in luminosity with increasing radius, transitioning to a slightly bluer color, implying the presence of younger stars and/or a lower metallicity. There is no discernable spiral arm structure or distinct dust lanes visible in this image. The overall shape appears close to circular, with only a slight elongation. There are no obvious signs of major mergers or significant tidal disturbances, although a hint of minor asymmetry may be present.
