The galaxy appears to be elliptical in morphology, with a relatively smooth light distribution and no apparent spiral arm structure. The color profile suggests a higher concentration of older stellar populations, as indicated by the redder hue towards the galaxy's core. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape. There is a suggestion of a faint outer halo or extended envelope, but this is difficult to discern with certainty. The galaxy shows no obvious signs of tidal interactions or major disturbances in its overall structure. A small, slightly bluer region is seen in the center of the galaxy, which might indicate a region of ionized gas. The light of the galaxy fades gradually into the background, with no sharp edges or cutoffs in its emission.
