The galaxy presents as a generally smooth, elliptical-like structure with a concentrated, bright central region, likely indicative of a galactic nucleus. The galaxy's light profile fades gradually from the core, suggesting a diffuse stellar distribution in its outer regions. There may be slight asymmetry to the shape, though this could be a result of the viewing angle, or potentially a minor interaction or disturbance. Overall, it appears as a relatively quiescent galaxy, with no strong evidence of ongoing major star formation within the visible spectrum.
