The galaxy appears to be an elliptical morphology, exhibiting a generally smooth and rounded structure. The central region displays a higher concentration of light, suggesting a prominent nucleus or core. Moving outward from the core, the light intensity gradually diminishes. There is a noticeable color gradient, with the central regions appearing more reddish, possibly indicating an older stellar population. Fainter, greenish hues are visible in the outer regions, which may be indicative of some ongoing or recent star formation, though at a low rate. There's no clear evidence of spiral arms, a distinct disk, or significant tidal disturbances. The galaxy's overall appearance suggests that it is a relatively relaxed system.
