The galaxy presents as a centrally concentrated luminous object with a generally smooth morphology. The core exhibits a bright, yellowish-white hue, transitioning to a reddish-orange towards the outer regions. There is a hint of ellipticity to the overall shape, appearing more rounded than highly elongated. While the central bulge dominates the light profile, there may be a faint, diffuse disk component contributing to the galaxy's overall extent, but this is not definitively discernable. No distinct spiral arms or bar structures are evident. There is no obvious presence of any major merging activity or tidal disruptions. The overall appearance suggests a relatively undisturbed system with potentially a dominant spheroid component.
