The galaxy presents as a centrally concentrated object, exhibiting a predominantly smooth morphology. The overall shape approximates a circular form, with a slight suggestion of ellipticity. The light distribution is centrally concentrated, with the luminosity gradually decreasing towards the outer regions. 

There's a subtle color gradient; the core appears slightly bluer than the outer regions, which exhibit a redder hue. This difference may indicate a younger stellar population in the central region. Possible tidal features or disturbances of a galaxy merger are present. No distinct spiral arm structures are detected, and its color suggests a redder stellar population in the outer regions. 
