The galaxy presents a generally smooth, elliptical morphology. Its color profile suggests a moderate redshift, evidenced by a more pronounced intensity in the redder bands compared to bluer wavelengths. This could indicate a greater proportion of older, redder stars compared to younger, bluer stars.

There's no prominent evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a concentrated central bulge, and a gradual fade in brightness moving outward from the core. There are some hints of minor distortions or asymmetries within the galaxy's structure, especially in the outer regions, potentially signaling past minor merger events or tidal interactions. Given the galaxy's apparent size and red color, it is possibly a massive galaxy.

The observed color gradient, from a slightly bluer central region to a redder outer halo, may indicate ongoing, albeit low levels of star formation in the central region.
