The galaxy presents a largely smooth, elliptical morphology. Its light profile suggests a dominant, spheroidal component. The color index, inferred from the provided data, indicates the presence of an older stellar population, with a relatively low ongoing star formation rate. The object appears moderately luminous, with a likely substantial stellar mass. Visual assessment does not reveal any prominent spiral arms or significant dust lanes. There is a mild elongation to the galaxy, but it is overwhelmingly round in shape. No major mergers are occurring in this system, though a slight asymmetry in the halo may indicate an ongoing minor disturbance.
