The galaxy appears as a relatively compact, single object with a fairly smooth overall morphology. There is a central, bright core that dominates the light profile, surrounded by a more diffuse, extended halo. Some minor asymmetry is visible in the halo, with a slight extension on one side, possibly indicative of a minor disturbance or interaction. The color of the core is predominantly blue-green, suggesting a population of hot, young stars or active star formation. The halo displays a broader range of colors including green and subtle red hues, potentially indicating a mix of stellar populations and/or dust content. There is little evidence of distinct spiral arms or other clearly defined features. The overall structure suggests that this galaxy might be an elliptical or lenticular galaxy, though a late-stage merger remnant cannot be ruled out.
