The galaxy presents as a centrally concentrated object with a generally smooth appearance. The light distribution suggests a dominant spheroid component. There is a notable absence of distinct spiral arm structures or prominent dust lanes. The overall shape is elongated, but not extremely so, trending more towards an elliptical morphology than a highly flattened disk. Subtle color variations are detectable, with a tendency toward bluer hues in the outer regions and a yellow/red core. There are no signs of intense tidal disturbances, or recent major merger activity. Faint disturbances may be present.
