The galaxy appears as an elongated, cigar-shaped structure, indicative of a highly elliptical morphology. It presents a generally smooth appearance, with a brighter, more concentrated region at one end. This brighter area may represent a galactic bulge or a region of enhanced stellar density. There may be evidence of a minor interaction or tidal disturbance to the galaxy, but the overall structure is relatively undisturbed, with no signs of ongoing major merging activity. The galaxy exhibits a color gradient along its major axis, suggesting possible variations in stellar populations or dust content along the galaxy's length, although it's quite faint overall. It is slightly resolved, but lacks significant detailed features. The galaxy presents a bluer color, indicating ongoing but minimal star formation activity, likely occurring at a low rate.
