The galaxy presents a predominantly smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The light distribution is centrally concentrated, with a bright core that gradually fades towards the outer edges. There is a slight elongation present, suggesting it is not perfectly spherical, tending towards a more circular shape.  Subtle variations in color might indicate differences in stellar populations, but these features are not prominent. There are no clear indications of ongoing major mergers or tidal disturbances in the immediate vicinity.
