The galaxy presents a primarily smooth and centrally concentrated morphology. The light profile appears relatively uniform, suggesting an elliptical or lenticular classification. There's a slight elongation observed, but it is close to round, possibly leaning towards an intermediate classification between round and cigar-shaped. There are no prominent spiral arms or bar structures discernible.

There is a hint of a faint, disk-like feature embedded within the galaxy, suggesting a possible past or ongoing merger event with a smaller system. The central region appears brighter than the outer regions, which fade into the background sky, implying a higher density of stars toward the galactic core. The overall color of the galaxy is yellowish-white, which indicates a population of older stars and a relatively low rate of recent star formation. There is no evidence of major tidal disturbances or ongoing merging activity. Overall, the galaxy appears to be a relatively quiescent system, potentially in a late stage of its evolution.
