The galaxy presents as a centrally concentrated, elliptical-like object with a smooth, diffuse appearance. There are no prominent spiral arms or distinct morphological features visible, such as bars or rings. The galaxy's light profile is relatively smooth, with a gradual decrease in brightness from the center towards the outer regions. The color appears to be predominantly yellowish-white, suggesting a stellar population that is moderately evolved. A faint, blueish halo or outer envelope surrounds the main body of the galaxy, which could indicate some low-level star formation. The overall structure implies a system dominated by older stars, likely a result of past mergers or interactions, with a smaller, more recent starburst event in the outer regions. Any ongoing merging activity is expected to be minor. 
