The galaxy appears as a centrally concentrated object with a roughly elliptical morphology. There is a bright, compact core, suggesting a possible active galactic nucleus or a dense stellar population. The galaxy’s light distribution seems relatively smooth, with little indication of distinct spiral arms or prominent dust lanes. The color profile of the galaxy suggests that it may contain a mix of stellar populations, with a relatively high mass. Faint irregularities can be seen in the galaxy's outer regions, indicating potential interactions with companion galaxies. The overall appearance implies that the galaxy has largely completed its major formation phases, presenting as a more mature system. The galaxy is more like an elliptical galaxy rather than a spiral.
