The galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, featureless morphology with no apparent spiral arms or distinct structures within the disk. The light distribution appears centrally concentrated with a bright, yellowish core that gradually fades outwards into a diffuse halo. The overall color suggests an older stellar population, with a possible absence of significant ongoing star formation. There is no evidence of tidal tails or strong gravitational distortions, indicating a quiescent state with no recent major merger activity. Subtle hints of a possible minor disturbance may be present in the outer regions, but it does not significantly disrupt the overall smooth appearance.
