The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated with a gradual decrease in surface brightness moving outwards from the core. The core region exhibits a yellowish hue, potentially indicative of an older stellar population, while the outer regions show some subtle bluer tinges, which might suggest the presence of younger stars or ongoing, albeit low-level, star formation. There's no clear evidence of spiral arms or a well-defined disk. The object is largely symmetrical, with no obvious signs of a major ongoing merger. Some small irregularities or minor disturbances are possibly present but not particularly prominent. The galaxy seems to be largely isolated in its immediate vicinity, with no clear indications of tidal interactions with neighboring galaxies. The overall roundness suggests that it is likely classified as an elliptical galaxy rather than a highly inclined spiral.