The galaxy presents a relatively smooth and centrally concentrated morphology, appearing elliptical or lenticular upon initial inspection. Its shape is neither perfectly round nor particularly elongated. There appears to be a slight asymmetry, which could indicate a minor interaction or disturbance. There is no obvious spiral arm structure or prominent disk. The galaxy exhibits a redder hue than some other objects in the field, which indicates an older stellar population and a lower rate of star formation. No major merging events are immediately apparent. There may be the presence of slight dust lanes or subtle features, but these are not very pronounced. Overall, this is an unperturbed, passively evolving system.
