The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The core exhibits a yellowish hue, suggesting an older stellar population likely dominated by red giant stars. Moving outwards from the center, the light gradually fades, transitioning to a more diffuse, bluish halo. There is no clear evidence of spiral arms or significant dust lanes. The galaxy appears to be an isolated system, with no obvious signs of tidal interaction or ongoing mergers. It appears to have some star formation activity, though it is most likely relatively low. The galaxy presents a moderate ellipticity, with an apparent axis ratio suggesting a deviation from a perfectly spherical shape. There are no readily apparent distortions in the overall morphology.
