The galaxy presents as a relatively smooth, elongated structure. The core region exhibits a concentrated, bright yellowish-orange hue, suggestive of an older stellar population. Moving outwards from the central bulge, the color gradually shifts to a more diffuse bluish-white, indicating the presence of younger stars. The galaxy lacks prominent spiral arm structures, appearing more lenticular in nature. The overall shape is somewhat cigar-shaped, with a moderate aspect ratio. The absence of significant morphological disturbances suggests it is not undergoing a major merger, though there may be evidence of a minor interaction or tidal feature. The galaxy displays a relatively high degree of symmetry.
