The galaxy exhibits a predominantly smooth morphology, with a central concentration of light that appears yellow-white, suggesting an older stellar population. A subtle, less defined blueish halo is visible surrounding the central region, possibly indicative of some ongoing star formation. The shape is mostly in between round and cigar shaped. There are no obvious signs of strong tidal interactions or major mergers. Minor disturbances appear possible, however no definitive sign. The galaxy appears relatively isolated, and the light distribution gradually fades away from the center, implying a lack of strong spiral arms or other prominent features.
