The galaxy presents as a centrally concentrated object, appearing largely smooth in structure. The light distribution suggests a primarily spheroidal morphology. There is a noticeable color gradient, with the core region exhibiting a yellow hue, transitioning to a reddish-orange towards the outer regions. The object exhibits a relatively circular shape, lacking any obvious spiral arms or bar-like structures. There are potentially minor tidal disturbances or interactions evident in the faint extensions around the primary galactic body, though the image resolution limits detailed analysis. There does not appear to be any clear evidence of active galactic nuclei activity or a significant amount of dust obscuration within the observed structure.
