The galaxy exhibits a generally smooth morphology, though some features suggestive of a disk are present. Its overall shape is elongated, with an approximate cigar-like appearance, indicating an elliptical or lenticular classification is probable. The central region displays a concentrated, bright, yellowish-orange hue, likely denoting an older stellar population. Fainter, more diffuse bluish areas extend from the central region along the major axis, potentially signaling regions of ongoing star formation. There is no obvious evidence of major mergers or significant tidal disturbances, though some minor asymmetries are seen within the fainter outer disk components which may be evidence of a minor interaction in the past. The overall color profile suggests moderate star formation activity relative to total mass.
