The galaxy presents a somewhat flattened, elliptical morphology. There appears to be a bright, relatively smooth central region, possibly indicative of a bulge or core. The galaxy's overall color profile suggests the presence of both young, hot stars exhibiting blue wavelengths, and a population of older, cooler stars contributing to the redder components. There is a faint halo surrounding the galaxy. Subtle distortions or irregularities are visible in the outer edges of the disk, with some signs of minor tidal disturbance possibly due to gravitational interaction with a nearby object or past merger event. Though the inner region appears smooth, the galaxy exhibits some features that suggest a degree of complexity beyond a purely elliptical system. 
