The galaxy presents as an elliptical or lenticular structure, exhibiting a relatively smooth and concentrated central bulge. The light distribution indicates a moderate degree of central concentration, with luminosity gradually decreasing outwards. The overall color of the bulge appears yellowish, suggesting a population of older stars. The disk component, if present, shows bluer colors compared to the bulge, indicating some ongoing star formation activity. The galaxy has a noticeable flattening, leaning towards a disk-like shape rather than a perfectly spherical one. It appears slightly disturbed, potentially indicative of a minor interaction or merger event in the past. No clear signs of strong tidal tails or disrupted morphology are visible, implying that if a merger occurred, it was either minor or happened far enough in the past to have relaxed.
