The galaxy appears to be a spiral galaxy viewed at a steep inclination. A prominent central bulge is observed, exhibiting a bluish-white hue, possibly indicating active star formation. The disk component presents a mottled appearance, suggesting a non-uniform distribution of stellar populations or dust. The galaxy exhibits faint, loosely defined spiral arms extending outward from the central bulge. Evidence of tidal disturbances or minor merger activity appears subtle, with only a slight asymmetry in the outer regions of the galactic disk. The galaxy's overall morphology suggests a system undergoing some form of interaction or internal rearrangement, though the specific nature of this activity requires further investigation.
