The galaxy presents as an elliptical morphology, exhibiting a high degree of smoothness throughout its structure. It appears nearly circular in shape, with a concentrated central region. The color profile indicates a population of older stars, suggested by the yellowish-orange hue of the galaxy core, surrounded by a cyan halo. There is no apparent spiral arm structure or significant dust lane obscuration. The object does not appear to be undergoing any major merging events or significant tidal disturbances. Overall, the galaxy seems to be a relatively undisturbed, evolved system.