The galaxy presents a generally smooth and elliptical morphology. Its core exhibits a high degree of luminosity, suggesting a dense stellar population and potentially an active galactic nucleus. The light profile appears concentrated towards the center, with a gradual fading in intensity towards the outer regions. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes. The overall color is predominantly yellowish-red, indicative of an older stellar population with a lower rate of ongoing star formation. There is no evidence of major mergers or significant tidal disturbances in the galaxy's structure. Minor asymmetry is observed in the outer edges of the galaxy.
