The galaxy presents as a luminous, somewhat elliptical object. The central region exhibits a concentrated brightness, suggesting a prominent galactic nucleus or bulge. Moving outwards from the core, the intensity of light diminishes gradually. The overall color profile of the galaxy appears yellowish-white, indicative of an older stellar population dominating the light output. There's a hint of bluer, potentially younger stars present in some of the galaxy's outer regions, though this is not a widespread feature. A faint, diffuse disk-like structure can be inferred, but it's not sharply defined. There is a possibility of some tidal interactions or minor mergers due to slight asymmetries. The galaxy does not show strong evidence of ongoing major star formation.
