The galaxy presents as a centrally concentrated object with a relatively smooth morphology. There is a slight elongation visible, deviating from a perfectly circular shape. The central region exhibits a bright, yellowish hue, potentially indicating an older stellar population. Fainter, more diffuse blue-greenish light extends outwards from the central region, possibly tracing areas of recent or ongoing star formation activity within a disk-like structure. There appears to be only a minor asymmetry in the outer regions of the galaxy, which may be due to a past or current minor gravitational interaction. Overall, the galaxy appears as a fairly evolved system with a mixture of stellar populations.
