This galaxy presents as an elongated, likely lenticular or edge-on spiral, morphology. The central bulge is prominent and appears relatively smooth with a bright, concentrated core. Faint, diffuse disk-like structure extends outward from the central bulge, characterized by a blueish hue indicative of more recent star formation in these outer regions. There is no visual evidence of strong dust lanes or prominent spiral arm structure from the image. The overall color gradient suggests a population shift, from older, redder stars in the central bulge, to younger, bluer stars in the outer disk. No signs of significant ongoing mergers or tidal disturbances are readily apparent.
