The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge is prominent and appears nearly spherical, exhibiting a concentrated luminosity. The light gradually decreases as it extends outward from the center, suggesting an absence of distinct spiral arms or features typically associated with disk galaxies. The color profile indicates a generally older stellar population, characterized by a yellowish hue in the central regions, transitioning to a slightly redder tone in the outer halo. There appears to be a subtle asymmetry in the outer regions, possibly indicative of a past or ongoing minor interaction. No significant dust lanes or star-forming regions are clearly discernible in the image. Overall, the galaxy's morphology points towards an evolved system, likely of substantial mass, that may be in the process of settling into a stable, spheroid-dominated configuration.
