The galaxy appears as a relatively compact object, exhibiting a red-shifted color profile. There's evidence of some disruption in its morphology, potentially indicating a minor interaction or disturbance. A slight asymmetry is visible in its overall shape, with a hint of distorted features that might be tidal tails or debris from a past merger. The central region displays a higher concentration of older stars and dust, while fainter, diffuse light suggests the presence of a more extended halo or envelope of stars. There is also a small but notable amount of active star formation.
