The galaxy presents as a relatively smooth, elliptical structure. There is a distinct central bulge with a high concentration of light, suggesting an older stellar population. The galaxy appears to be mostly featureless, lacking prominent spiral arms or a significant disk component. It shows a yellowish hue in the central region, likely indicative of older, redder stars. The outer regions exhibit a gradual decrease in luminosity and a slightly bluer tint, potentially indicating the presence of younger stars or some level of ongoing star formation. There are subtle hints of possible minor disturbances or interactions, though no major merger events are immediately apparent. The overall shape is largely spheroidal, with a mild deviation towards a cigar shape.
