The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that transitions into a more diffuse outer region. The color gradient suggests the presence of an older stellar population, particularly in the central region, indicated by a yellower hue which then appears to fade into a blue tinge as the stellar population decreases to the outer portion of the structure. There's no obvious spiral arm structure or distinct dust lanes visible. The overall morphology suggests a galaxy that is largely spheroidal in shape, with a high degree of symmetry. There is no indication of ongoing major merger activity, although some minor disturbances may be present.
