The galaxy presents a moderately diffuse appearance with a centrally concentrated core. The overall shape is somewhat irregular, deviating from a perfectly elliptical form. There is a suggestion of a possible tidal tail or minor disturbance extending outwards. The color distribution indicates that this is likely a relatively low mass system with ongoing but somewhat subdued star formation. The inner region seems to be a bit more actively forming stars than the halo. There is no clear evidence of a prominent disk structure or spiral arms, suggesting it could be a transitioning spiral or an irregular dwarf galaxy. There is a slight color variation across the galaxy, with a hint of reddish tones in the outer regions.
