The galaxy presents as a somewhat symmetrical elliptical or lenticular form. There is a central bulge that appears luminous and concentrated, gradually fading into a less dense halo. The overall color profile leans towards the redder end of the spectrum, suggesting a population of older stars. No distinct spiral arm structures are visible, implying a lack of significant ongoing star formation. The edges of the galaxy appear smooth, showing no signs of major tidal disturbances or ongoing mergers.
