The galaxy presents as a generally smooth object, with a suggestion of a central bulge. The overall shape approximates an elliptical form, appearing somewhat elongated but predominantly rounded. There is an absence of clear spiral arm structures or prominent dust lanes. Color gradients across the galaxy suggest a population of older stars, trending towards redder hues in the central regions. The galaxy exhibits a relatively low star formation rate. The estimated stellar mass is substantial. There is no strong evidence of ongoing major merger activity, although minor tidal disturbances cannot be completely ruled out.
