This galaxy exhibits a somewhat elliptical morphology, though not perfectly spherical. The central region presents a bright, concentrated luminosity, suggesting a dense stellar population, potentially an older bulge. Moving outward, the light profile appears to diffuse, indicating a more extended, though not clearly defined disk.

The color distribution across the galaxy shows variations. The central region exhibits a yellow-green hue, possibly indicating older stellar populations. The outer regions appear more reddish, which could be due to the presence of dust or ongoing star formation. There is some visible structure suggesting a possible disturbance or interaction, though a definitive merging event is not readily apparent.
