The galaxy presents a generally smooth appearance, with a slightly elongated morphology. The light distribution suggests an elliptical or lenticular classification. The central region exhibits a concentration of luminosity, potentially indicating an older stellar population with minimal ongoing star formation. There is a slight color gradient, with the central regions appearing more yellow-red in comparison to the outer edges which may contain some blueish areas. There is evidence of some disturbance in the structure, however no tidal tails or signs of merger activity are clear in the image. Based on the light profile, the effective radius of the galaxy is moderately small. The overall structure seems generally undisturbed.