The galaxy presents as an elliptical morphology, viewed at an angle that indicates a slight flattening. The central bulge is prominent and exhibits a bright, concentrated luminosity, suggesting a high stellar density, potentially including an older stellar population. A fainter, more diffuse halo surrounds the core, extending further along the major axis than the minor axis. There appears to be a subtle color gradient from the center outwards, with the central regions exhibiting a more yellow/white hue, transitioning to a bluer tinge in the outer regions of the disk. There may be some slight dust features going on near the outer edge of the disk, but it is hard to say. The disk is generally smooth and lacks the distinct spiral arm structure commonly observed in spiral galaxies.
