The galaxy presents as a slightly elongated, disk-like structure with a smooth, centrally concentrated bulge. The light profile indicates that this is likely an early-type galaxy, potentially an elliptical or lenticular, with a high Sersic index indicating strong central concentration. The color gradient suggests the presence of an older stellar population dominating the bulge, as indicated by a yellowish hue. The galaxy shows a relatively smooth morphology, with no apparent signs of active star formation regions or significant dust lanes. There is little evidence of spiral arm structure. The overall structure and color suggest a passively evolving galaxy.
