The galaxy presents as a relatively smooth, elongated structure. A central bulge is readily apparent, exhibiting a yellowish-white hue suggestive of an older stellar population. Surrounding the bulge is a faint, diffuse disk. The disk is not particularly well-defined, showing a bluer tint on the outer edges, indicative of potential ongoing star formation regions. The overall morphology suggests a disk galaxy, possibly of an intermediate type between elliptical and spiral, where the spiral arms are not clearly distinguished. There may be some minor irregularities or disturbances along the disk, but no major merging events or significant tidal features are visible. The galaxy appears to be relatively isolated and undisturbed.
