The galaxy presents as a spiral, with a relatively bright central bulge. The spiral arms are well-defined but tightly wound, displaying a bluish hue, indicative of ongoing star formation. The disk appears moderately inclined relative to our line of sight, contributing to its elliptical appearance. A weak bar structure appears to be present within the central region. The bulge constitutes a moderate fraction of the overall galactic light. The dust lanes are not particularly prominent.
