The galaxy presents as a somewhat elliptical, diffuse object, with a central bulge that appears more concentrated and brighter than its outer regions. The colour profile suggests a generally older stellar population. The light distribution exhibits a smooth, symmetrical structure with no prominent spiral arms or strong morphological disturbances. The presence of faint reddish tinges at the outer edges of the galaxy could indicate ongoing star formation. The image resolution limits a more precise morphological classification, but the overall structure is consistent with an early-type galaxy, possibly an elliptical or lenticular type. There is a slight possibility of minor disturbances.