The galaxy presents as a centrally concentrated object with a generally smooth appearance. Its light profile suggests a relatively homogenous stellar population throughout the majority of its structure. The central region exhibits a bright, slightly elongated core. The overall shape of the galaxy appears more rounded than elongated, though a subtle, cigar-shaped feature cannot be fully ruled out. There are no obvious signs of spiral arm structures or significant dust lanes. Additionally, there is no strong evidence of recent or ongoing major merging activity, although the possibility of minor past interactions or disturbances cannot be discounted based on this image alone.
