The galaxy presents an elongated, cigar-like morphology, suggesting it could be an elliptical galaxy viewed at an angle, or a highly inclined spiral galaxy. The light distribution appears relatively smooth and centrally concentrated, with a gradual decrease in surface brightness towards the edges. The central region exhibits a brighter, more luminous area, likely indicating a higher density of stars or the presence of an active galactic nucleus. There's a slight hint of bluer colors in the outer regions. This suggests the presence of younger stars and possibly ongoing star formation, although the overall color suggests an older stellar population dominates. There does not appear to be any signs of strong tidal distortions or obvious merger activity. 
