The galaxy presents as a relatively smooth, centrally concentrated object. Its light profile suggests a spheroidal morphology. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a color gradient, transitioning from a bright, yellowish-white core to a fainter, slightly redder outer region. This color gradient could indicate an aging stellar population concentrated in the galaxy's center, with a younger population more sparsely distributed in the outskirts. There is a slight distortion of the shape, but it seems to be an elliptical shape, rather than an actively merging galaxy. This galaxy has a very faint star forming region.