The galaxy presents a generally smooth, elliptical morphology. A central bulge region is visible, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Fainter, bluer light surrounds the core, likely indicating regions of more recent star formation. The galaxy appears relatively isolated. While not perfectly smooth, there is no strong evidence of ongoing major mergers, but subtle disturbances cannot be ruled out based on this image alone. The overall size of the galaxy is substantial, suggesting a mature system. The color profile indicates a mix of stellar populations, with older stars concentrated towards the center and younger, bluer stars distributed throughout a less-defined disk-like structure.
