The galaxy presents as a relatively smooth, lenticular-like structure with a slight elongation, appearing somewhat cigar-shaped. There is a subtle color gradient, suggesting older stellar populations. The galaxy exhibits a central concentration of light, possibly indicating a small bulge. There is no evidence of a pronounced disk or spiral arms; any structure present is rather diffuse and indistinct. The morphology is indicative of a galaxy that has largely ceased significant star formation, supported by the subtle color. There is no clear indication of recent or ongoing major mergers. There might be a minor disturbance in the overall shape, possibly an early stage merger, but further investigation would be needed to confirm this.
