The galaxy presents a somewhat diffuse appearance, with a central region that appears brighter and more concentrated. Its morphology suggests a classification leaning towards a smooth galaxy, possibly an elliptical or lenticular type. There is a hint of disc like structure, though not sharply defined. The central bulge exhibits a yellowish hue, potentially indicating an older stellar population. Faint extensions of diffuse light are observed surrounding the central region, which could be indicative of a halo or tidal features resulting from past interactions. Star formation appears minimal to absent within the galaxy, based on the overall color distribution and apparent lack of prominent blue regions associated with young, hot stars. There are signs of minor disturbances on the edges, which are indicative of potential tidal interactions with other galaxies. 
