The galaxy presents as an elongated, cigar-shaped system with a prominent central bulge. The core exhibits a concentrated luminosity gradient, suggesting a high density of stars and possibly a supermassive black hole at its center. Moving outwards from the core, the luminosity decreases gradually, and there is a visible disk structure that is not fully resolved, likely due to its distance. The disk is oriented at an angle relative to our line of sight. The galaxy’s overall color appears reddish-yellow, indicative of an older stellar population and a reduced rate of star formation within the disk. There may be some minor disturbances in the disk structure, such as slight asymmetry. No distinct spiral arms or prominent dust lanes are clearly visible at this resolution. The galaxy does not show any signs of a major merging event.
