The galaxy presents as an elongated, cigar-shaped structure. Its overall form is relatively smooth, with the light intensity concentrated towards the center. There appears to be a subtle color gradient, shifting from a slightly redder hue in the central bulge region to a bluer tint in the fainter, extended outer regions. The galaxy appears relatively isolated with no obvious signs of ongoing or recent major mergers or tidal interactions. The light distribution indicates a mostly dispersed structure.
