The galaxy appears as a central, luminous object with a somewhat elliptical morphology, exhibiting a moderate degree of smoothness. The central region is characterized by a bright, concentrated light profile, potentially indicating a substantial stellar population. The light extends outward, diminishing in intensity toward the edges of the galaxy. There is a subtle color gradient discernible; the central regions seem to possess a bluer hue, while the outer edges may exhibit a slight reddish tint. Hints of asymmetry are present, with a possible minor disturbance or interaction occurring on one side of the galaxy. No distinct spiral arms or bar structures are readily apparent. Overall, the galaxy presents features consistent with an intermediate-mass system undergoing a moderate level of star formation.
