The galaxy presents as an elongated, ellipsoidal structure. It appears relatively smooth, with a concentrated central region that gradually fades into the surrounding halo. The light distribution suggests a lack of distinct spiral arms or other prominent features, such as dust lanes or bright star-forming regions. The color profile is predominantly reddish-yellow, indicating an older stellar population. There is no visual evidence of ongoing major merging events, though minor disturbances cannot be ruled out based on this single image. The galaxy exhibits a noticeable ellipticity, appearing cigar-shaped rather than circular.
