The observed galaxy presents as a highly inclined disk galaxy, viewed nearly edge-on from our vantage point. It exhibits a prominent central bulge, appearing bright and concentrated. The bulge displays a smooth, rounded morphology. The galactic disk is thin and elongated, extending significantly from the central bulge. The color profile suggests a relatively old stellar population, particularly within the bulge, which is consistent with a reduced rate of star formation. There are no visible spiral arm structures or significant dust lanes obscuring the galaxy's light. There appears to be a faint hint of disturbance or minor irregularity in the disk's structure on one side, possibly due to past interactions or minor tidal effects.
