The galaxy presents a generally smooth morphology, with a hint of a disturbed structure. The color profile suggests a mixed population of stars. The central region exhibits a subtle blue-ish hue, potentially indicating ongoing or recent star formation activity, or a slightly younger stellar population. The overall light distribution is moderately concentrated, but without a distinct nucleus. There appears to be a faint tidal tail or bridge extending away from the main body, hinting at a possible past or ongoing interaction or merger. The object is relatively compact in size, and appears to have a relatively low star formation rate.
