This galaxy presents a largely smooth and somewhat elliptical morphology. It exhibits a concentrated central bulge that emits strongly in yellow wavelengths. This bulge transitions smoothly into a fainter, less defined outer region. This outer region displays a subtle color gradient shifting towards redder hues. There is minimal evidence of distinct spiral arm structures or significant dust lane features within the galaxy's morphology. The overall appearance suggests an evolved stellar population. There appears to be only minor disturbances, if any, of the galaxy's shape, indicating that it is most likely not currently undergoing any major merging activity.
