The galaxy appears to be an elliptical type, characterized by a generally smooth and featureless morphology. It presents as a centrally concentrated object with light diminishing towards the outer edges. The elongation is significant, with the galaxy appearing cigar-shaped. There is a subtle color gradient visible, with a slightly bluer hue in the central region transitioning to redder tones towards the outskirts. No distinct spiral arms or other disk-like structures are observed. There is no obvious evidence of a major ongoing merger, although subtle asymmetry might suggest past gravitational interactions or minor disturbances. The galaxy exhibits a moderate apparent magnitude, suggesting a relatively high luminosity. The effective radius is of moderate size. The overall appearance is consistent with a galaxy dominated by an older stellar population, but with a small amount of recent star formation.
