The galaxy presents as an elongated, somewhat cigar-shaped structure, suggesting an elliptical morphology. The light distribution appears smooth and centrally concentrated, with no distinct spiral arms or prominent features visible. The color gradient transitions from a bright, slightly yellowish core to a more diffuse, reddish outer halo. This color profile hints at an older stellar population in the central regions, potentially indicating diminished star formation activity. The overall form suggests a system that is relatively undisturbed, lacking evidence of major mergers or tidal interactions in its recent history, although there may be evidence of a minor disturbance.
