The galaxy appears as an elliptical system with a smooth, concentrated light profile. There is a prominent central bulge exhibiting a yellowish hue, suggesting a population of older stars. The overall shape is elongated, exhibiting a cigar-shaped morphology. Subtle color gradients are visible, with the outer regions appearing slightly bluer. The absence of obvious spiral arms or significant dust lanes suggests a relatively quiescent galaxy, with a low rate of ongoing star formation. No signs of major mergers are apparent in the galaxy's morphology. There may be minor disturbances in the outer regions of the galaxy.
