The galaxy presents a somewhat elliptical morphology, with a concentrated central bulge. The light distribution appears relatively smooth, with some indication of a possible disk structure extending outwards from the core. A faint blue tinge is observed in these outer regions, possibly indicating some star formation activity. There are suggestions of minor tidal disturbances or asymmetries in the outer structure, though these are not highly pronounced. Redder regions are sparsely visible, possibly indicating areas of older stellar populations. The overall appearance suggests a galaxy that is transitioning from a spiral or irregular morphology towards a more elliptical, quiescent state.
