The galaxy appears as a centrally concentrated object, with a predominantly smooth light distribution. The overall morphology suggests an elliptical or lenticular type. There is a slight elongation observed, deviating from a perfectly circular shape. Faint, extended regions of light are visible, suggesting a diffuse halo or outer envelope. The galaxy exhibits a color gradient, with a more yellow/white core and slightly bluer outer regions. There is no immediately obvious indication of distinct spiral arms or prominent dust lanes. Based on its morphology and color profile, this galaxy appears to be a relatively massive system with moderate ongoing star formation. There is some slight asymmetry to the light distribution.