The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The core region exhibits a yellowish-white hue, suggestive of an older stellar population. There is a noticeable, yet subtle, extension of light emanating outwards from the central core, indicative of a bulge and possibly a disk component viewed at an angle. The outer regions of the galaxy fade gradually into the background, lacking sharp boundaries or prominent spiral arm structures. There is a slight elongation in the galaxy's shape, deviating from a perfectly circular form, possibly suggesting an elliptical morphology or the presence of minor tidal disturbances. Based on the luminosity, this appears to be a massive galaxy undergoing some star formation. There appears to be a slight disturbance in the overall shape and structure, which could be indicative of a possible minor merger event in the past. 
