The galaxy presents a largely smooth morphology, with little in the way of discernible spiral arms or other distinct features. The light distribution is concentrated towards the center, suggesting the presence of a central bulge. The object's shape appears closer to being in between round and elliptical, with some deviation from a perfectly circular form. There's an absence of any signs that would suggest any major ongoing mergers. The color indices suggest that the galaxy contains both older stellar populations. The blue light suggests active or recent star formation, but the contribution from redder wavelengths indicates the presence of older stars too. The inferred stellar mass suggests that this is a relatively massive system, while the inferred star formation rates indicate it is a galaxy with relatively low star formation activity.
