The galaxy appears as a centrally concentrated object with a generally smooth profile. It exhibits a moderate degree of ellipticity, appearing somewhat elongated but not dramatically cigar-shaped. The core region is brighter and shows a yellowish-orange hue, suggestive of an older stellar population. A fainter, more diffuse halo surrounds the core, displaying a subtle gradient in color, transitioning to a slightly bluer tone in the outer regions. There is no evidence of strong spiral arm structure or distinct star-forming regions visible within the image. The overall impression is that of a relatively evolved galaxy with subdued star formation activity. There may be some minor irregularities in the outer halo suggesting a possible past or ongoing interaction, but they are not pronounced.
