The galaxy appears as a relatively smooth, elliptical-like structure. The central region displays a concentrated, reddish hue, possibly indicating an older stellar population or significant dust obscuration. Extending outwards from the core, a more diffuse, greenish glow is observed, suggestive of younger, hotter stars and potential ongoing star formation in the outer regions. The galaxy exhibits a slight elongation, deviating somewhat from a perfectly circular form, though no obvious spiral arm structures or significant morphological disturbances are readily apparent. Based on its size, it appears to be a moderately sized galaxy, likely a significant but not a massive system. There is some faint indication of recent disturbance in the outer disk, but its generally regular shape makes it an unexceptional galaxy.
