The galaxy presents as a fairly smooth, diffuse object with an estimated effective radius of approximately 6 arcseconds. The central region is significantly brighter, exhibiting a high degree of luminosity, suggesting a concentrated nucleus. The overall color profile appears to be relatively red, with a notable gradient towards the outer regions, where a faint, disk-like structure can be tentatively identified. There is a suggestion of possible minor disturbance in the morphology, potentially indicating a past or ongoing interaction, but the galaxy predominantly exhibits a relaxed, non-merging structure. 
