The galaxy presents as a relatively smooth, amorphous structure. It exhibits a somewhat elliptical morphology, displaying a moderate elongation. The color profile appears to be dominated by redder wavelengths, with a hint of green and blue, suggesting a population of older stars and possibly some ongoing but low levels of star formation. There is no apparent spiral arm structure or prominent dust lanes visible in this image. The galaxy does not appear to be undergoing a major merger, though there might be some minor disturbance in its overall structure.
