The galaxy appears to be a relatively small, elliptical or lenticular galaxy with a noticeable disk. The galaxy's core appears bright and concentrated, suggesting a significant stellar population and possible presence of an active galactic nucleus. The disk appears smooth and relatively featureless, with little evidence of spiral arms or star-forming regions. There is a slight suggestion of a warped or disturbed morphology. The object does not look like a merger, however there is a chance for a minor disturbance, which could imply recent or ongoing interactions. The galaxy exhibits a color gradient, with the central regions appearing redder and the outer regions appearing bluer. This may indicate differing stellar populations, where the bluer regions have younger stars. There appears to be no clear dust lane visible. 
