This galaxy presents as a relatively smooth, elongated, and cigar-shaped structure. The color profile suggests a more pronounced blue hue at the outer edges, indicative of younger stellar populations and potentially ongoing star formation in the galactic disk. The central bulge appears yellower and redder, implying the presence of older, redder stars. A faint, dusty structure may be embedded within the disc, but the resolution limits a more definitive assessment. No major disturbances or tidal features are clearly visible, suggesting the absence of recent major merger events, though minor interactions cannot be ruled out. Overall, this galaxy appears to be a disk galaxy, likely an edge-on or highly inclined spiral, with evidence of differing stellar populations between the bulge and the disk.
