The observed galaxy exhibits a pronounced spiral structure. While partially obscured and somewhat faint, discernible spiral arms extend from a relatively bright central bulge. The arms appear somewhat flocculent, displaying a patchy distribution of star-forming regions characterized by a bluish hue. The presence of dust lanes is suggested, particularly near the central region, though detailed observation is limited by the image resolution.

The bulge appears moderately sized relative to the overall galaxy disk. Its color suggests an older stellar population. The winding of the spiral arms is moderate. The disk component shows a general lack of extreme distortion, suggesting the galaxy has likely not undergone a recent major merger. 

Based on the distribution of light, a stellar bar is likely present.
