The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core region exhibits a bright, yellowish-white color. Moving outwards, the color transitions to a bluer hue in the surrounding regions, suggesting the presence of a younger stellar population. There's a slight elongation, but overall, the galaxy appears relatively round. No obvious spiral arms or strong morphological disturbances are visible. The galaxy appears to be relatively isolated, with no immediately apparent signs of ongoing or recent major merger activity.
