The galaxy appears as a centrally concentrated, luminous object with a smooth morphology. There is an elliptical shape to the object, with the light intensity decreasing gradually from the core outwards. A yellowish hue is present towards the center, suggestive of an older stellar population and diminished recent star formation. The galaxy's outskirts appear fainter and bluer, indicating the presence of younger, hotter stars, though these are not a dominant feature. There is no visual evidence of prominent spiral arms or significant dust lanes. No signs of major mergers or tidal disturbances are obvious in this image, although subtle irregularities cannot be ruled out without further data. The object appears relatively isolated.
