The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a predominantly elliptical morphology. It appears largely featureless, with no obvious spiral arm structure or strong dust lanes visible in this image. The color profile suggests an older stellar population, trending towards redder hues. The isophotes are generally rounded, indicating a high degree of rotational symmetry. There is no strong evidence of recent major merger activity or tidal distortions in the immediate vicinity of the galaxy. The galaxy possesses a bright central bulge. Some minor disturbances may be present.