The galaxy presents as a centrally concentrated, elliptical morphology. The light profile exhibits a smooth, gradual falloff from the core, suggesting a high degree of sphericity. The core itself displays a yellowish hue, indicative of a stellar population dominated by older, redder stars. There is no discernible spiral arm structure or significant dust lane obscuration. Faint, diffuse extensions are visible along the major axis, hinting at a slightly elongated shape, but these features are subtle. No distinct merging events or major tidal disturbances are evident in the immediate vicinity. Overall, the galaxy appears to be a relatively isolated, well-formed elliptical system. The faint bluer light at the edges indicates a small amount of on-going star formation is possibly occurring.
