This galaxy presents a largely smooth, elliptical morphology. There is a concentrated central bulge exhibiting a yellowish hue, suggesting a relatively older stellar population compared to what would be expected in active star-forming regions. The galaxy is characterized by a lack of prominent spiral arms or a distinct disk structure. The overall roundness appears to be elliptical, but not extremely elongated. There is no visual evidence of any major ongoing merging events or significant tidal disturbances, indicating it is likely a relatively relaxed system. The galaxy appears to be undergoing only a low level of star formation. The general color and structure are consistent with a massive system with suppressed star formation.
