The galaxy presents as a disk galaxy, observed at a high inclination relative to our line of sight, appearing somewhat cigar-shaped. The central bulge exhibits a bright, concentrated luminosity, suggesting a high stellar density in that region. A subtle color gradient is discernible, with the central region exhibiting a yellowish-white hue that transitions to a reddish tint towards the outer regions of the disk. No distinct spiral arm structures are immediately apparent in the image, likely due to the angle of inclination and the limited resolution. The disk exhibits a relatively smooth texture, indicating a lack of prominent dust lanes or regions of intense star formation.
