This galaxy presents a generally smooth and rounded morphology. There is little evidence of spiral arms or a prominent disk structure; rather, it appears more spheroidal in shape. The galaxy exhibits a fairly concentrated central region that transitions smoothly outward, with no sharp edges. The light distribution is generally uniform, though there appear to be some very faint, diffuse features extending outwards. These appear disturbed, but with a relatively low light level. The overall color of the galaxy appears to be in the yellow-red range, suggesting a population of older stars and a relatively low star formation rate. There is very little blue light or evidence of young, hot stars. The galaxy does not show signs of any recent or ongoing major merger activity.
