The galaxy exhibits a generally smooth morphology, appearing largely featureless in this image. Its shape is somewhere between round and elongated, leaning slightly more towards an intermediate form. The primary color is a yellowish-orange, indicating an older stellar population. There is no readily apparent disk structure. Weak signs of a minor disturbance are present, but there is no major merger or significant tidal disruption. The galaxy possesses a significant mass suggesting a substantial stellar population. Its star formation rate is relatively low for its size, leading to a higher mass of old stars as opposed to new stars being formed.
