The galaxy presents as a smooth, elliptical morphology, exhibiting a concentrated central bulge. A disk component is either absent or not clearly discernible within the limitations of the image resolution. The galaxy has an overall roundish appearance, though it does deviate slightly towards a more elongated, cigar-like shape. There's no evidence of any major disturbances. The nucleus appears bright and relatively compact, possibly indicating active star formation. A faint color gradient is noticeable, shifting from a yellowish core to a somewhat bluer halo, which may suggest different stellar populations within these regions. Overall, the galaxy appears to be well-isolated, with no immediately obvious signs of interaction or merging events.
