The galaxy presents as a slightly elongated, elliptical-like structure, though not a perfect ellipse. The light distribution appears relatively smooth across the galaxy, showing no significant spiral arm features or distinct dust lanes. There is a central concentration of light, suggesting the presence of a bulge. The color profile indicates a yellow/orange hue in the central region, potentially indicative of an older stellar population. Fainter bluish colors at the outer edges may hint at a younger stellar population or ongoing star formation in those regions, though this is less certain. There is no obvious sign of strong tidal disturbances or ongoing mergers. The galaxy appears relatively isolated and undisturbed.
