The galaxy presents a distinctly elongated, cigar-shaped morphology. It exhibits a central bulge region that appears relatively smooth and dominant, emitting light that is notably yellower in color, suggesting an older stellar population. The outer regions of the galaxy appear less defined, gradually fading into the background sky. There is a faint, diffuse disk structure surrounding the central bulge, but no distinct spiral arms or other prominent features are discernible. The smoothness suggests a lack of significant ongoing star formation within the disk. There is no evidence of any major mergers or tidal disturbances affecting the galaxy's overall structure.
