The galaxy presents a face-on spiral morphology, exhibiting a moderately sized bulge with tightly wound spiral arms. The central bulge appears luminous with a yellow-white hue, suggesting a significant population of older stars. The spiral arms extending from the bulge display a mixture of blue and yellow regions, indicating both ongoing star formation and older stellar populations. The disk component is somewhat obscured in areas, possibly due to dust lanes or patchy star formation. There appears to be a bar structure across the central region of the galaxy. The galaxy does not appear to be undergoing any major merging events, however, a minor disturbance within the arms could be the result of interactions with another galaxy or uneven distributions of stellar populations.
