The galaxy presents as a relatively smooth, elliptical-like object. There is a central bulge that exhibits a concentrated luminosity, and a more diffuse, extended halo. The light distribution suggests a higher concentration of older stellar populations. The color profile indicates a blue shift, potentially signaling active but moderate star formation. Although the galaxy appears mostly undisturbed, there may be some subtle, minor irregularities in the outer halo, possibly suggesting past minor interaction. The object's overall morphology is transitioning to a more spheroidal shape.
