The galaxy presents as a somewhat elongated, elliptical object. There is an apparent color gradient across the galaxy, with the upper portion displaying a yellow hue, possibly indicating an older stellar population. The lower portion of the galaxy exhibits a bluer color, suggesting the presence of younger, hotter stars and potentially ongoing star formation. The main body of the galaxy appears relatively smooth with no obvious signs of spiral arms or distinct morphological features. There appears to be a slight asymmetry in the light distribution but no strong evidence for tidal tails or mergers. Based on this information it could be classified as a lenticular galaxy and is of significant size and luminosity.
