The galaxy presents as a spiral type, observed at an intermediate inclination. Two spiral arms are clearly discernible, winding moderately around a central bulge. A bar structure appears present and defined, extending through the bulge region. The bulge itself seems relatively small compared to the overall disk size. The spiral arms show broad dust lanes. There is no evidence of any ongoing major merging events, although a possible minor tidal interaction cannot be entirely ruled out. The light profile suggests ongoing star formation.
