The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution indicates a higher density of stars towards the center, gradually decreasing outwards. There is a hint of bluer hues at the edges of this galaxy, possibly indicating regions with slightly more active star formation. The overall color profile leans towards the redder end of the spectrum, implying an older stellar population. There is no apparent spiral arm structure or significant dust lanes visible. The galaxy seems to be relatively isolated, with no obvious signs of major tidal disturbance or interaction with other galaxies.
