The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellowish-orange hue, suggesting an older stellar population. The galaxy appears elongated, with the major axis significantly larger than the minor axis, resulting in a cigar-like shape. There is no strong evidence of spiral arms or a prominent disk structure. The outer regions of the galaxy fade gradually into the background sky, indicating a diffuse halo. No obvious signs of recent merger activity or significant tidal disturbances are detected. Overall, the galaxy appears to be a relatively quiescent, early-type system.
