The galaxy presents as a relatively smooth, elliptical morphology. Its light profile is centrally concentrated, exhibiting a radial decrease in surface brightness without apparent spiral arm structures or a distinct bulge. The color appears to be a fairly uniform yellowish-red hue, suggesting an older stellar population, which typically correlates to a small range of star forming properties. There is no obvious indication of ongoing major merger activity or significant tidal disturbances, with the galaxy maintaining a fairly regular, rounded shape. It's likely a mature system, undergoing little to no recent interactions.
