The galaxy presents a generally smooth, elliptical morphology with an overall blue-white hue. A bright central bulge is apparent, gradually fading into a less luminous, extended halo. The core appears nearly spherical, with the outer regions becoming slightly elongated. There are no clearly defined spiral arms or significant dust lanes visible, suggesting a relatively evolved stellar population with limited ongoing star formation. Subtle color variations within the galaxy hint at some structural complexities but these are largely smoothed out. There is no obvious evidence of a major merger event, although there could be minor disturbances affecting its structure.
