The galaxy presents a centrally concentrated light profile, appearing as a roughly elliptical, though somewhat irregular, morphology. The core region exhibits a yellowish-white hue, suggesting an older stellar population. There is a subtle gradient in color outward from the center, with the outer regions appearing slightly bluer, possibly indicating ongoing star formation or a younger stellar population there. Hints of a very faint, diffuse disk structure appear to be present, though it is not well-defined, and the light is smoothly distributed, suggesting no prominent spiral arms or bar features are visible. There is some indication of slight irregularity in the galaxy's overall shape, which could potentially indicate a past or ongoing minor interaction or disturbance. Overall, the galaxy appears relatively smooth and evolved.
