The galaxy presents a somewhat elliptical morphology with a bright, concentrated central bulge that transitions smoothly into a more diffuse outer region. The color profile exhibits a gradient; the core appears to be a yellow-white hue, suggestive of an older stellar population, whereas the outer regions show hints of bluer tints, potentially indicative of ongoing or recent star formation. Faint spiral arm structures can be discerned emerging from the central region and wrapping around the galaxy. There is a slight asymmetry in the overall structure of the galaxy, perhaps due to past or ongoing minor gravitational interactions. It exhibits a degree of smoothness, but there is also indication of disc structure.
