The galaxy appears as a somewhat elongated structure with a brighter, more concentrated central region. The light distribution suggests a roughly ellipsoidal shape when viewed from our perspective. The galaxy exhibits a relatively smooth appearance overall, with a fuzzy or diffuse outer region that gradually fades into the background. Within the central region, there appears to be a subtle color gradient, shifting towards redder hues, possibly indicating an older stellar population in the core. The outer regions show hints of bluer colors, suggesting ongoing, albeit potentially low-level, star formation. There is some visual evidence of minor disturbances or irregularities in the galaxy's structure, potentially indicative of past interactions or internal processes.
