The galaxy presents as an elliptical morphology, exhibiting a smooth and centrally concentrated light distribution. The core appears bright and yellow, possibly indicating a population of older stars. The outer regions of the galaxy gradually fade into the background sky, suggesting a diffuse stellar halo. There are no apparent spiral arms, dust lanes, or significant star-forming regions visible. The overall color suggests a relatively low rate of star formation and a generally evolved stellar population. There is no obvious indication of any merger activity or significant tidal disturbances. The galaxy appears largely undisturbed.
