This galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated bulge with a gradual decrease in luminosity moving outwards. The galaxy presents with an overall rounded morphology, showing minimal evidence of a disk structure or significant spiral arms. There are no immediately obvious signs of ongoing major merger activity or substantial tidal disturbances, although subtle asymmetries or faint features cannot be entirely ruled out at this resolution. The color profile suggests a dominant population of older stars, indicating a relatively low rate of current star formation.
