The galaxy presents as a relatively smooth, elongated structure. Its shape is reminiscent of a cigar or spindle, suggesting an elliptical morphology viewed at an angle. A central bulge appears to be the brightest region, exhibiting a yellowish hue. The outer regions are fainter and appear somewhat bluer. This may be due to older stars populating the bulge and disk with younger stars dominating the outer regions. There may be a faint indication of a disk component. There is no apparent strong evidence of spiral arms or significant dust lanes. The galaxy appears isolated, with no obvious signs of interaction or tidal features.
