The galaxy appears to be an elliptical galaxy with a smooth, spheroidal morphology. The light profile shows a central bulge with a gradual decrease in luminosity moving outwards, suggesting an even distribution of stars and a lack of significant spiral arms or distinct features. The galaxy exhibits a yellowish-orange hue, which would indicate an older stellar population with a relative lack of ongoing star formation. There are faint hints of bluer tones within the outer regions, suggesting there may be younger, hotter stars present, but this is not immediately apparent. The galaxy shows an elliptical shape that is elongated with the brightness concentrated toward its center. There does not appear to be evidence of any recent major merging events, such as tidal tails or disturbed morphology.