The galaxy presents as a smooth, centrally concentrated object. Its morphology is dominated by a bulge, appearing roughly elliptical in shape. The central region exhibits a bright, yellowish hue, suggestive of an older stellar population. The outer regions fade into a dimmer, bluish color, possibly indicating the presence of some younger, bluer stars, but the overall smooth appearance does not suggest ongoing, significant star formation. There are no apparent signs of spiral arms, bars, or significant dust lanes. No major disturbances or interactions with other galaxies are visible. The galaxy appears relatively isolated.
