The galaxy presents a primarily smooth morphology, with an overall elliptical shape. It is not perfectly round, appearing slightly elongated, but not significantly cigar-shaped. The central region exhibits a concentrated luminosity, appearing bright and yellowish, potentially indicating an older stellar population. A subtle color gradient can be observed moving outwards from the center; the inner regions display warmer hues, gradually shifting toward cooler colors in the outer regions. There is no obvious indication of spiral arm structures or significant dust lanes. No apparent major merging activity or significant tidal disturbances can be seen, but there may be a minor disturbance to the structure.
