The galaxy presents as an inclined spiral with a notable central bulge. The bulge exhibits a yellow-white hue, indicating a population of older stars. The spiral arms are not well-defined, appearing flocculent and somewhat disrupted. There appears to be evidence of ongoing or recent star formation, highlighted by faint blueish regions tracing the spiral structure. Patches of what appear to be dust lanes or obscured regions are also visible within the spiral arms. Overall the galaxy demonstrates moderate levels of disturbance.
