The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears yellowish in color. The surrounding region displays a smoother profile with slightly bluer hues at the edges. The galaxy is elongated, appearing cigar-shaped, and exhibits little evidence of strong spiral arm structures or active star formation regions in the disk. There are subtle irregularities indicating a possible minor disturbance or interaction, though a major merger event seems unlikely. The overall morphology suggests a galaxy with an older stellar population.
