The galaxy presents a generally smooth and elliptical morphology. It appears largely spheroidal with a high degree of central concentration. The color profile indicates a dominant population of older stars, lending a yellowish-red hue to the galaxy’s core. There are no prominent spiral arms or significant dust lanes visible. Faint, diffuse extensions surround the core, indicating a gradual decrease in stellar density towards the outer regions. Based on its shape, it appears as a single, non-interacting system, with no clear evidence of tidal distortions or ongoing mergers. The overall structure suggests a lack of significant recent star formation activity.
