The galaxy presents as a centrally concentrated object, exhibiting a predominantly smooth morphology. There is little discernable internal structure, such as spiral arms or a prominent bar. The overall shape appears elliptical, tending towards roundness rather than a highly elongated, cigar-like form. A radial gradient in color is observed, with the core region displaying a yellowish-white hue, suggesting a population of older stars. The outer regions of the galaxy gradually fade into a bluish halo, potentially indicating the presence of a younger stellar population or some low-level star formation. There are no obvious signs of recent major mergers or significant tidal disturbances, although subtle irregularities in the outer isophotes might hint at minor interactions in the past. The galaxy's size seems relatively modest, suggesting a moderate scale in terms of its stellar mass and overall luminosity.
