The galaxy appears as a centrally concentrated, moderately luminous object. It exhibits a generally smooth morphology, with a slight elongation in shape. The core region is characterized by a bright, relatively unresolved central component. The color profile suggests a mixture of stellar populations; the central region shows hints of older, redder stars, while the outer regions appear to be bluer, potentially indicating the presence of younger stars or ongoing star formation. There is no clear evidence of spiral arm structure or a prominent disk component. Subtle irregularities or minor disturbances can be observed in the outer regions of the galaxy, possibly indicating past or ongoing minor merger events. Overall, the galaxy appears to be a transitioning system, perhaps an intermediate stage between a spiral and an elliptical galaxy.
