The galaxy presents as a relatively compact object. It appears largely spheroidal in shape. The light distribution suggests a smooth stellar population, potentially an elliptical morphology. The core region exhibits a higher concentration of luminous material, which could indicate an active galactic nucleus or a dense central star cluster. Overall the galaxy appears to be relatively red in color, which could indicate an older stellar population or significant dust obscuration. No distinct spiral arms or other prominent disk-like features are apparent in this observation.
