The galaxy presents a generally smooth morphology with a concentrated central bulge. The shape appears moderately elliptical, transitioning from round to slightly elongated. There is a suggestion of a faint, diffuse disk component surrounding the bulge, though its boundaries are ill-defined and lack prominent spiral arm structures. Overall the galaxy appears to be a relatively massive galaxy with a small amount of star formation. There are hints of minor tidal disturbances or asymmetries within the extended halo, but they are subtle and do not indicate an active major merger event.
