The galaxy presents as a disk galaxy, viewed at a moderately oblique angle. The central bulge region appears bright, with a yellowish hue. Fainter, more diffuse light extends outwards from this core, tracing a flattened, elliptical shape. The overall morphology suggests that it is a relatively smooth and undisturbed system, showing no signs of any major mergers or significant tidal interactions. The gradient from the core to the outer edges suggests that this disk is somewhat spheroidal rather than a pure disk. The presence of more light in the redder bands coupled with a general lack of blue light might be due to a population of older stars, and very little present star formation.
