The galaxy presents a largely smooth and elliptical morphology. It is centrally condensed with a bright, yellowish core, indicative of an older stellar population. The galaxy exhibits a relatively symmetrical shape, appearing mostly round. The outer regions gradually fade into the background, and the disk fraction appears low, meaning we do not observe a typical spiral pattern. There appears to be little to no evidence of ongoing major merging activity or significant tidal disturbances within the visible structure. The colors present are mostly a more aged yellowish color, and the light emitted from the core of this galaxy is more redshifted when compared to the outer parts.
