The galaxy appears as a centrally concentrated luminous object, with a smooth, somewhat elliptical morphology. The core region exhibits a reddish hue, suggesting a population of older stars. A faint, extended halo surrounds the central region, displaying a gradient from reddish hues near the center to greenish and bluish tints in the outer regions. This color variation may indicate ongoing star formation in the outskirts, or differences in stellar populations. There is no evidence of strong spiral arm structure or a prominent disk from this vantage point, but a slight asymmetry is apparent. The overall smooth appearance suggests it is a relatively evolved system, though perhaps with some recent or ongoing low-level star formation. The galaxy does not appear to be undergoing any major merger events or significant tidal disruptions based on the image.
