The galaxy appears as a cigar-shaped, relatively smooth object with a slightly disturbed morphology. The central region exhibits a brighter, concentrated luminosity, possibly indicative of an older stellar population. Moving away from the center, there is a noticeable decrease in light intensity and a change in color. One end of the galaxy is distinctly bluer, suggesting ongoing star formation. The overall structure indicates an elliptical galaxy with some evidence of a disk-like component. There may be minor disturbances or interactions affecting its shape. Overall, the galaxy exhibits a moderate mass and exhibits low to moderate star formation. 
