The galaxy presents as a lenticular structure, with a smooth, largely featureless central bulge. The galaxy exhibits an intermediate ellipticity, with the overall shape appearing neither perfectly spherical nor highly elongated. There is a suggestion of a faint disk component, although the image resolution makes it difficult to ascertain distinct spiral arm structures or significant dust lanes. The light distribution is centrally concentrated, fading gradually outwards from the core. A possible minor tidal disturbance appears to be present, or perhaps a smaller galaxy in the process of merging. The galaxy displays a moderately high luminosity. The color indices suggest that there is ongoing, or recent star formation activity, though it is not a strong signature. Overall, this galaxy appears to be a relatively evolved system, potentially transitioning from a spiral to an elliptical morphology.
