The galaxy presents as a fairly symmetrical elliptical, exhibiting a relatively smooth morphology with minimal discernible features. The color profile shows a distinct concentration of light towards the red end of the spectrum, hinting at an older stellar population. There are no distinct spiral arms or a pronounced disk structure visible. The galaxy appears to be mostly homogenous without significant internal structures. The overall shape is close to circular but may show signs of elongation. There is no obvious evidence of a significant merger event. Any disturbances appear minor, if present at all.