The galaxy presents as a centrally concentrated object, appearing largely smooth in morphology. It exhibits a slight elongation, deviating marginally from a perfectly circular form. The light distribution suggests a bulge-dominated structure, with a gradual decline in surface brightness moving outwards. The galaxy appears to be a yellowish hue, with hints of redder tones in the outer regions. There is no apparent spiral arm structure or dust lane features visible within the galaxy. Given the smooth appearance and color, the galaxy appears to have an older stellar population and a relatively low current star formation rate. There is a suggestion of a very minor disturbance in the lower part of the image, although it is unlikely to be a merger.
