The galaxy presents a relatively smooth, elliptical morphology. It exhibits a centrally concentrated light profile, appearing brightest at its core, with the light gradually fading towards the outer regions. The overall color is indicative of an older stellar population, with a yellow-orange hue dominating the image. There is minimal evidence of distinct spiral arms or significant dust lanes. The galaxy shows a slight elongation, deviating somewhat from a perfectly circular shape, suggesting a moderate degree of flattening. There does not appear to be any signs of major tidal disturbances or ongoing mergers in this image, although I do observe a minor disturbance on one edge of the galaxy. The image suggests the object is a rather massive galaxy with a relatively low star formation rate.
