The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. The central region displays a brighter, more intense luminosity, suggesting a higher density of stars and possibly a central supermassive black hole. Moving outward from the core, the luminosity gradually decreases, transitioning into a fainter, more diffuse halo. There is a subtle, irregular structure surrounding the brighter core with slightly bluer tendrils, hinting at some possible spiral arms or a disk that is not very well defined. The galaxy exhibits a moderate ellipticity, appearing somewhat round but deviating slightly from a perfect circular shape. There is no apparent interaction with other galaxies, with no tidal tails or strong distortions visible, possibly indicating a relatively isolated system. The color profile reveals a central region that is yellow, grading to red outwards, which may suggest an older stellar population dominating the core with a small presence of younger, bluer stars in the surrounding areas.
