The galaxy presents as a roughly elliptical shape with a smooth, diffuse appearance, possibly an early-type spiral or lenticular. Its color profile suggests a concentration of older stars towards the central bulge, indicated by a yellowish hue in the core region. The outer regions exhibit a bluer color, inferring the presence of younger stellar populations and some star formation, although it appears subdued. There are no pronounced spiral arms or features indicative of intense star-forming regions, instead, the arms appear weak and flocculent. The galaxy shows some evidence of minor disturbances. The overall morphology hints at a galaxy that is transitioning from a more active star-forming state to a more quiescent phase.
