The observed galaxy presents an elliptical morphology. It appears elongated, exhibiting a cigar-like shape, with a smooth light distribution. The central region is brighter and appears to be slightly more red-shifted, suggestive of an older stellar population concentrated in the core. The outer regions display a bluer hue, potentially indicating the presence of younger stars, although the light is faint and blending into background sky. There is no clear evidence of spiral arms or significant dust lanes, and no obvious sign of a major merger event or tidal disturbance. The galaxy seems relatively isolated and undisturbed.
