The galaxy appears as a centrally concentrated object with a relatively smooth overall appearance, although some faint, irregular features are present. The core region exhibits a yellowish hue, indicative of an older stellar population. Emanating from this central region is a faint, diffuse spiral structure or possible tidal arm extending towards the right side of the image. Patches of blueish light are scattered throughout, indicating regions of recent star formation. The galaxy appears to be relatively massive, and exhibits a low star formation rate. There is evidence of potential interaction or disturbance based on the irregular features. The central bulge appears to dominate the galaxy's overall light profile. The galaxy is approximately 17 kpc across.
