The galaxy presents as a somewhat smooth, elliptical object. It exhibits a centrally concentrated bulge, which appears yellowish to reddish in color, suggesting an older stellar population. Moving outward from the center, a bluer hue becomes more prominent in the disk, suggestive of ongoing star formation. The galaxy appears elongated, with an axis ratio indicating that it is not perfectly circular but rather somewhat cigar-shaped. No distinct spiral arms are visible, nor is there any obvious evidence of a major merger event. There might be minor disturbances within the halo, but that may also be due to image artifacts. Overall, the galaxy appears to be an intermediate-mass system with a moderate redshift, displaying characteristics of both evolved and actively star-forming regions.
