The galaxy presents as a lenticular or edge-on spiral galaxy with a smooth central bulge. It has an elongated, cigar-like shape. The color gradient transitions smoothly from a yellowish-orange core to fainter, bluish hues at its outer edges, suggesting the presence of a mixed stellar population with older stars concentrated centrally and younger stars in the outer regions. There is evidence of a faint disk structure, though its features are subtle. No significant dust lanes or active star-forming regions are clearly visible within the galaxy. There are no signs of recent or ongoing mergers or tidal disturbances. Overall, the galaxy appears to be a relatively isolated system in a late stage of its evolution.
