The galaxy presents as a somewhat rounded, centrally concentrated structure. Its overall morphology leans toward smooth, showing minimal signs of distinct spiral arms or a well-defined disk. The central region exhibits a brighter, yellowish hue, possibly indicating an older stellar population or a higher concentration of stars. Moving outwards from the center, the color shifts toward a bluer tone, suggesting the presence of younger stars or ongoing star formation in the outer regions. There might be a faint, extended halo or envelope surrounding the main body, although this is difficult to discern due to the image resolution. There are no strong indications of any major mergers or significant tidal disturbances.
