The galaxy presents a relatively smooth morphology, dominated by a central bulge that appears nearly spheroidal. The bulge exhibits a yellowish hue, suggesting an older stellar population. A faint, extended disk is visible, surrounding the central bulge. The disk appears bluish, hinting at the presence of younger, hotter stars and ongoing star formation, though not at a particularly high rate. The galaxy does not display any strong spiral arm structure or other significant features indicating a recent major merger. There may be evidence of some minor disturbance in the outer regions of the disk, possibly indicating interaction with a smaller satellite galaxy or tidal effects. The overall shape of the galaxy is closer to in between round and elliptical.
