The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology, trending towards a round shape. There is a bright, yellowish central bulge, which diminishes in intensity outwards. The outer regions show a fainter, bluer hue, suggesting the presence of younger stellar populations compared to the bulge. There's a possible, subtle indication of a faint disk structure. No significant tidal features or evidence of major merging activity are immediately apparent, although a minor disturbance cannot be entirely ruled out due to the resolution.