The galaxy presents an overall elliptical morphology, with an elongated, cigar-like shape. The central region exhibits a concentrated, yellowish-white glow, suggesting a significant population of older stars. Moving outward from the core, the galaxy displays a change in color. The central region seems to be surrounded by a ring of greenish-blue light, which might indicate a more active region of star formation.

The galaxy is relatively smooth in appearance, with little evidence of spiral arm structure. However, there are some subtle color gradients and slight asymmetries, which hint at potential interactions or minor disturbances. It appears to be in a relatively isolated environment, as no other large galaxies are immediately apparent in the image. The redder, fainter features on the outer edges could signify dust absorption, or a population of older, redder stars. There is no obvious sign of any major merger or intense starburst activity, just possibly minor disturbance.
