The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The core region exhibits a bright, yellowish-white luminosity, suggesting a high density of older stellar populations. The radial color gradient shifts from the yellowish-white core to a slightly redder hue in the outer regions, indicating a possible change in stellar population or dust content. No distinct spiral arm structure or prominent dust lanes are apparent. There is a slight deviation from perfect ellipticity, but no major disturbance or signs of ongoing merging events are visible. Overall, this galaxy appears to be a quiescent, well-formed system, likely an elliptical galaxy.
