The galaxy presents as a single, largely homogenous structure. The morphology is dominated by a smooth, elliptical shape, appearing nearly round with minimal discernible features such as spiral arms or a distinct galactic bar. A central bulge is readily apparent, exhibiting a significantly higher luminosity and a yellow hue. The luminosity fades gradually from the core outward, with the outer regions displaying a redder color profile. There is no evidence of significant tidal disturbances, ongoing major mergers, or pronounced star formation regions based on the image. The overall appearance is consistent with an evolved galaxy that contains a notable population of older stars.
