This galaxy presents a predominantly smooth, elliptical morphology. The light distribution appears centrally concentrated, lacking significant spiral arm structures or prominent dust lanes. The galaxy exhibits a moderately round shape, showing only slight elongation. The color profile suggests an older stellar population, with a yellow-red hue dominating the galaxy's central region. There is no strong visual evidence of ongoing major merger activity, although some minor disturbance cannot be ruled out given slight irregularities in its overall shape. The galaxy appears to be a relatively isolated system, lacking any immediately apparent companion galaxies or tidal features that would indicate recent strong gravitational interactions.
