The galaxy appears as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. Its color profile suggests an older stellar population, exhibiting a yellowish hue, most pronounced towards the center of the galaxy. There is little evidence of spiral arms or dust lanes, indicating that the galaxy is likely an early-type galaxy, possibly an elliptical or lenticular galaxy viewed from a distance. The outer regions of the galaxy appear to fade gradually into the background sky, suggesting a diffuse stellar halo. The galaxy shows no signs of any recent major mergers or significant tidal disturbances.
