The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology with no prominent spiral arms or disk structure discernible at this resolution. The light distribution indicates a concentrated central bulge that fades gradually outwards toward the edges of the galaxy. The shape is elongated, more akin to a cigar shape as opposed to perfectly round, with a slight tilt relative to the line of sight. There are no signs of major ongoing merger events or significant tidal disturbances; however, a subtle asymmetry could indicate a possible minor interaction in its past. Color gradients within the galaxy suggest a variation in stellar populations, with a slightly redder core potentially indicating older stars or higher dust content. 
