The galaxy presents as an elongated, somewhat cigar-shaped object with a notable color gradient. The central region displays a more concentrated, yellowish-orange hue, suggesting an older stellar population and/or significant dust obscuration. The outer regions exhibit a bluer tint, indicative of more recent star formation activity. The galaxy appears relatively smooth, with a high concentration of light in its center, with little evidence of distinct spiral arms or other major structural features. There are no prominent tidal tails or other indications of a recent major merger event. A slight asymmetry is apparent along its major axis, potentially hinting at minor interactions or internal disturbances. The light distribution fades gradually towards the edges, indicating a less defined boundary.
