The galaxy presents an overall smooth morphology. Its shape is elongated, appearing as an ellipse. It shows a concentrated central bulge with a yellow-gold hue, suggesting an older stellar population. There is a faint disk extending from the central bulge, displaying a bluish tint, which indicates the presence of some younger, hotter stars and regions of active star formation, although the proportion seems low. No spiral arms or significant dust lanes are clearly discernible in this image. There are no signs of a major ongoing merger, though a minor disturbance cannot be completely ruled out based on the galaxy's asymmetry.
