The galaxy presents as a centrally concentrated object with a slightly elongated, cigar-shaped morphology. The core exhibits a yellowish-white hue, suggestive of an older stellar population. Extending outward from the core, a more diffuse halo is visible, displaying a gradient towards redder hues and lower surface brightness. There is some subtle evidence of potential disturbance in the outskirts, particularly a slight asymmetry in the halo's distribution. Overall, the galaxy appears to be a relatively massive system.
