The galaxy appears to be a somewhat compact and luminous object, with an elliptical morphology. The galaxy exhibits a generally smooth light distribution, lacking prominent spiral arms or other distinct features. There is some evidence of a slight distortion or tidal feature, suggesting a possible minor interaction or past merger event. The galaxy displays a strong central bulge, with a gradual decrease in luminosity toward the outer edges. Color gradients suggest a moderate amount of ongoing or recent star formation activity within the galaxy, possibly concentrated in the central regions. The color index indicates it may be at intermediate redshift. There may be a slight roundness to the galaxy with a small chance of cigar shaping. It is possible that there is no merging activity occuring. 
