The galaxy presents as an elliptical or lenticular system with a dominant, smooth light profile. The central bulge appears prominent and exhibits a yellowish-red hue, indicative of an older stellar population. Moving outward from the core, the galaxy displays a fainter, bluish disk. The disk has a less defined structure, showing minimal spiral arm features and a more diffuse light distribution. The galaxy's overall shape is somewhat elongated, appearing more "in between" than completely round, tending toward a cigar shape. There is no obvious evidence of ongoing major mergers or tidal disturbances from other galaxies, suggesting it's a relatively isolated system, though the presence of minor disturbances cannot be ruled out. 
