The galaxy presents as a lenticular or possibly an elliptical type, exhibiting a notably elongated, cigar-like morphology. The central bulge is prominent and appears relatively smooth, displaying a yellowish-white hue suggesting an older stellar population. The outer regions of the galaxy show a gradual decrease in luminosity, fading into the background sky. There's a subtle hint of a disk-like structure extending from the central bulge, potentially indicating some rotational dynamics. Faint blueish regions are observed along the periphery, implying the presence of some younger, hotter stars, though these features are not strongly defined. Overall, the galaxy appears relatively undisturbed, without significant signs of ongoing mergers or tidal interactions.
