The galaxy appears as a relatively smooth, elliptical-like structure with a dominant, centrally concentrated bulge. Its overall color is yellowish, suggesting a stellar population dominated by older, redder stars, which would imply a low current rate of star formation. There is no clear evidence of spiral arms or a disk structure. The light distribution is fairly even and diffuse, with no distinct features like bright star-forming regions or dust lanes. Based on the morphology, the galaxy appears to be undisturbed, with no obvious signs of ongoing or recent merger activity or significant tidal distortions. The size of the object is moderately extended, but it appears relatively compact.
