The galaxy presents as a generally smooth object with a somewhat elongated, cigar-shaped morphology. The central region exhibits a bright, concentrated core indicative of a significant stellar population density, likely dominated by older stars. Moving outwards from the core, the light intensity gradually diminishes, suggesting a decreasing stellar density.

The overall color profile appears to be slightly reddish-yellow, implying a population of evolved stars and a low ongoing star formation rate. There is a hint of a faint disk-like structure or possibly a spiral arm segment visible, but the lack of distinct features suggests this galaxy is mostly elliptical or lenticular in nature. There is no evidence of any major ongoing mergers or significant tidal disturbances. Overall, the galaxy appears to be a relatively undisturbed system, likely nearing the end of its star-forming lifecycle.
