The galaxy presents as a moderately bright object with a generally smooth, elliptical morphology. It exhibits a gradual fading in surface brightness from the center outwards, lacking any distinct spiral arm structures or prominent dust lanes. The overall color is slightly reddish, suggestive of an older stellar population and a relatively low rate of current star formation. The shape appears mostly round, with a subtle deviation from perfect circularity. There is no obvious indication of any ongoing major merger activity or significant tidal disturbances in the immediate vicinity. The galaxy appears relatively isolated, with no nearby galaxies showing signs of strong interaction.
