The galaxy presents a smooth, featureless morphology. The light distribution suggests an elliptical or lenticular type. A slight elongation is observable, but not pronounced. There appears to be a centrally concentrated bulge with a gradual decline in surface brightness moving outwards. The color profile shows a yellowish hue centrally with a slight shift toward redder colors in the outer regions. This color gradient could indicate an older stellar population dominating the galaxy's composition, with possibly less ongoing star formation activity. There is no evidence of spiral arms, dust lanes, or any significant tidal disturbances. The overall impression is of a relatively quiescent and evolved system.
