The galaxy presents as a slightly elongated, smooth object. The central region exhibits a bright, concentrated bulge, appearing a yellowish-orange hue. This color likely indicates an older stellar population dominating the core. Extending outward from the core, the galaxy appears to have a diffuse disk, with hints of bluer regions, perhaps indicative of more recent star formation, though it is subtle. There may be a very faint, almost imperceptible spiral structure, however, the feature is not prominent. The overall structure suggests a relatively evolved system. The galaxy does not exhibit any obvious signs of a major merger, although there could be a very slight disturbance in its overall symmetry, that may suggest a minor interaction, however, this may also simply be the effect of the viewing angle. The galaxy is moderately sized with the light appearing to be primarily centrally located.