This galaxy appears to be a lenticular or early-type spiral, with a generally smooth light distribution. The central bulge is bright and concentrated, transitioning gradually into a fainter, more diffuse disk. There is little evidence of strong spiral arm structure or prominent dust lanes, suggesting a relatively quiescent state of star formation. The overall color is somewhat blue, particularly in the disk, indicating the presence of some younger, hotter stars. The morphology of the galaxy seems to exhibit a slight elongation, not fully spherical but not highly flattened either, possibly indicating an intermediate stage between elliptical and spiral galaxies. There are hints of minor disturbances or irregularities in the outer regions, which may be evidence of past or ongoing interactions with smaller galaxies, however this galaxy appears to be generally isolated and undisturbed.
