The galaxy presents as a lenticular or edge-on spiral type. It exhibits a notably elongated, cigar-like morphology, suggesting a substantial disk component viewed at a high inclination angle. The central bulge is subtly brighter than the surrounding disk. The color gradient transitions from a yellowish-orange core to a slightly bluer hue towards the outer regions, hinting at a radial change in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars potentially populating the disk. There is no distinct evidence of prominent spiral arm structure, but some faint disk features may be present. No signs of significant tidal disturbance or ongoing major merger activity are readily apparent.
