The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth morphology. The light profile appears to decline steadily from the core outwards, lacking any distinct spiral arms or a prominent disk structure. The dominant color is a yellow-orange hue in the central region, potentially indicative of an older stellar population, and suggesting relatively low on-going star formation. The overall shape is somewhere in between round and elliptical. There is no strong evidence of a major merger. A very slight distortion in the outer regions might suggest minor tidal interactions with another galaxy.
