The galaxy presents as an elliptical morphology, characterized by a centrally concentrated bulge exhibiting a yellow-orange hue, possibly indicating an older stellar population. The luminosity decreases radially outwards from the core. The outer regions of the galaxy show a bluer tint. No distinct spiral arm structures are visible, suggesting a relatively smooth distribution of stellar mass. There are no distinct regions of recent star formation observed, supporting the dominance of an older stellar population within the galaxy. The overall shape is neither perfectly spherical nor significantly elongated, suggesting a moderate degree of ellipticity. There is no visible evidence of ongoing mergers or tidal disturbances.
