The galaxy presents as an elongated, cigar-shaped structure, appearing largely smooth in texture with a slight asymmetry in its overall form. Its light profile suggests a centrally concentrated bulge region, which gradually diffuses outwards into a more extended disk. A subtle color gradient is discernible, transitioning from a bluish hue in the outer regions of the disk to a slightly redder tint closer to the central bulge, potentially indicative of differing stellar populations and star formation activity. There may be an indication of a faint, disturbed structure on one side of the galaxy, which may imply some kind of interaction or tidal feature. The observed morphology is consistent with an early-type spiral or lenticular galaxy, with evidence of moderate to low levels of ongoing star formation.
