The galaxy presents as an elongated, disk-like structure, observed nearly edge-on. A central bulge is apparent, exhibiting a yellowish-orange hue, suggesting a population of older stars. The disk component shows a slight blue tint, indicative of ongoing star formation. Some dust lane obscuration is visible in the disk, causing slight irregularities in light intensity. No distinct spiral arm structure is readily discernible at this resolution. There is no indication of any major merger activity, though some minor asymmetry exists which could indicate a past merger event or tidal interaction.
