The galaxy presents as a somewhat smooth and elliptical structure, though with subtle irregularities suggesting possible interactions or internal dynamics. There appears to be a bright central bulge, exhibiting a yellowish hue, which likely indicates an older stellar population. Diffuse, blue-tinged regions are visible in what could be interpreted as a disk, although it lacks defined spiral arms. These bluish areas suggest the presence of younger, hotter stars and ongoing star formation. The galaxy exhibits a moderate degree of elongation, appearing somewhere between a circular shape and a cigar shape. There is a potential hint of disturbance in the galaxy's morphology, which could be indicative of a minor gravitational interaction or merger event. Overall, the galaxy is relatively compact with its light concentrated towards the core.
