The galaxy presents a generally smooth morphology, with a dominant, centrally concentrated bulge region exhibiting a yellowish hue. This suggests a population of older stars. Faint, diffuse extensions are visible, hinting at a disk-like structure, or possibly tidal interactions. There is evidence of an area of mild disturbance off to the right, showing a faint orange color. The galaxy is neither distinctly elliptical nor a well-defined spiral, but presents a moderately rounded form. There may be some ongoing, but minor, gravitational interactions.
