The galaxy presents as a single, relatively smooth object with a concentrated central bulge and an extended halo. The core exhibits a yellowish-orange hue, suggesting an older stellar population. The outer regions appear fainter, with a subtle color gradient indicating a possible difference in stellar ages or composition compared to the core. The overall shape is elliptical, leaning toward a slightly elongated form. There are no prominent spiral arms or dust lanes visible. Minor disturbances in the overall smoothness may be indicative of past interactions or minor merging events. Based on these characteristics, the galaxy is likely a massive elliptical with a low rate of star formation.
