The galaxy appears as a somewhat elliptical, diffuse object. A concentrated, bright central bulge dominates the galaxy's morphology. The bulge exhibits a yellowish hue, possibly indicating an older stellar population. Fainter, bluer light emanates from what might be a surrounding disk component, although the disk structure is not sharply defined. There is little evidence of spiral arms, suggesting that any present are either tightly wound or indistinct. Overall, the galaxy seems relatively smooth, with no apparent signs of major mergers or significant disturbances. Subtle asymmetries might indicate minor gravitational interactions.
