The galaxy presents a moderately elongated morphology. It exhibits a central concentration of light that appears relatively smooth. Fainter, somewhat diffuse extensions are observed outwards. Overall, the galaxy shows a general lack of strong features or spiral arms, and the overall form suggests a system that is neither perfectly elliptical nor a well-defined spiral. The color profile indicates a redder center, transitioning to somewhat bluer hues in the outer regions. This color gradient may suggest differences in stellar populations, with older, redder stars concentrated in the core and younger, bluer stars populating the outer regions where star formation might be occurring.
