This galaxy presents as a spiral type with a central bulge that transitions into a disk. The bulge appears moderately sized and exhibits a yellowish hue, suggestive of an older stellar population.

Prominent spiral arms extend outwards from the central region. These arms display a bluish tint indicative of ongoing star formation, likely due to the presence of younger, hotter stars. The arms show a somewhat disrupted structure on one side. On the opposite side, it is difficult to determine the structure due to its closeness. 

The overall morphology hints at possible gravitational interactions or a minor merger event, potentially influencing the irregularity observed in the spiral arm structure. The galaxy exhibits a slight tilt relative to the observer's line of sight.
