The galaxy presents a generally smooth and rounded appearance, with a slight deviation from perfect circularity. It exhibits an elliptical morphology, being more elongated than spherical but not displaying a pronounced disk structure. There is some evidence of minor internal structures, although no distinct spiral arms or bars are visible. The galaxy's core appears bright and relatively compact, suggesting a concentration of stars or possibly an active galactic nucleus. The overall color suggests a relatively mature stellar population, with a moderate degree of star formation. There are very faint hints of disturbed morphology suggesting the possibility of interaction, but it would be minor. The galaxy exhibits a substantial mass, likely consisting of a large number of stars, gas, dust, and possibly a central supermassive black hole. The galaxy appears to have a notable rate of ongoing star formation, indicating some reservoir of gas available for stellar birth.
