The galaxy presents a largely smooth morphology, suggesting an elliptical classification. The light distribution is concentrated towards the center, with a radial decrease in brightness. Its overall shape appears close to round. There is no discernible evidence of spiral arms or a prominent disk structure. The color profile is relatively uniform, exhibiting a yellowish-red hue, consistent with a population of older stars. There is no obvious indication of recent or ongoing major mergers or tidal disturbances, though a minor disturbance cannot be completely ruled out. The galaxy appears to be a relatively quiescent system with a low star formation rate.
