The galaxy presents as an elliptical morphology with a smooth light distribution. The central region exhibits a bright, concentrated core. The overall color appears to be yellowish-white, suggesting an older stellar population dominating the galaxy's light. There is a slight elongation in its shape, deviating from a perfectly circular form, tending towards a cigar shape. No distinct spiral arms or dust lanes are discernible. There are no indications of any major ongoing merger activity or significant tidal disturbances. The galaxy appears relatively isolated. Based on the color and lack of visible star formation features, it can be inferred that the star formation rate within the galaxy is low.
