The galaxy appears to be a relatively smooth, elliptical type, exhibiting a concentrated central bulge. It has a generally rounded morphology, with minimal signs of disk-like features or significant distortions. The light distribution is centrally concentrated. The galaxy's color appears to be skewed towards the redder end of the spectrum, suggesting an older stellar population with less active star formation. There's no strong visual evidence of ongoing major mergers, though subtle asymmetries might hint at minor disturbances in its past.
