The galaxy presents as an elliptical morphology, exhibiting a smooth and largely featureless profile. The light distribution suggests a high degree of central concentration, with the core region appearing significantly brighter than the outer regions. A color gradient is present; the central bulge exhibits a yellowish hue, potentially indicative of an older stellar population. Moving outward, the color becomes slightly bluer, but this change is subtle, implying a relatively homogenous stellar population throughout. There is no discernible dust lane or spiral arm structure. The overall shape is slightly elongated, deviating minimally from a perfectly circular form, but mostly round. There is no evident signs of any major disturbances or interactions with other galaxies. 
