The galaxy exhibits a predominantly smooth morphology with a centrally concentrated bright core, potentially indicative of an active galactic nucleus or a significant stellar bulge. There is some evidence of faint, diffuse features extending outward from the core, possibly a faint disk or tidal disturbances. These features lack distinct spiral arm structure or well-defined edges. The light distribution suggests a relatively evolved system with a significant fraction of older stellar populations, as supported by the color profile where the core is bluer and outer extensions appear redder. There is an indication of a minor disturbance within the galaxy's structure which may suggest a past or ongoing minor merger event.
