The galaxy presents as a relatively compact object with a smooth, elliptical morphology. Its color profile skews towards the redder end of the spectrum, with a prominent central bulge exhibiting a yellowish-orange hue. There is minimal evidence of spiral arm structure or significant star-forming regions within the visible light wavelengths. The galaxy appears undisturbed, lacking tidal tails or other indications of recent major merger events. A slight elongation suggests it is not perfectly spherical, with some deviation toward a more lenticular shape. Overall, the galaxy appears to be a mature system dominated by an older stellar population, consistent with a relatively low star formation rate.
