The galaxy presents as a relatively smooth, lenticular-like structure with an elongated, cigar-shaped morphology. Its color profile indicates a redder hue overall, suggesting an older stellar population with diminished ongoing star formation. A slight central brightening is noticeable, possibly indicating the presence of a galactic bulge. There are no prominent spiral arms or dust lanes visible. The galaxy appears relatively isolated, with no immediately apparent signs of major tidal interactions or ongoing mergers, although there may be some evidence of minor disturbances.
