The galaxy appears as a moderately bright, compact object. It exhibits a generally smooth morphology with a slightly elliptical shape, showing no strong signs of spiral arm structure or a pronounced central bulge. The color gradient suggests a bluer core region potentially indicative of younger stellar populations or active star formation, surrounded by a somewhat redder halo, which is consistent with a population of older, redder stars. There might be very minor disturbances or distortions in its shape, but the galaxy appears mostly undisturbed, with a very small possibility of a minor merger. Overall, the galaxy presents as a relatively high mass object with a moderate rate of star formation.
