The galaxy presents as a spiral type, viewed at an angle slightly off from face-on. The central bulge appears significant in size, dominating the overall luminosity profile. It exhibits a yellowish-white hue, suggesting an older stellar population. Spiral arms are present and relatively tightly wound, tracing outwards from the central bulge. These arms display a clumpy texture, indicative of star-forming regions. There does not appear to be a strong bar feature present. Subtle distortions may be present within the disk, suggestive of a possible minor interaction or merger event in the galaxy's past. The overall color profile indicates ongoing star formation, but with a considerable population of older stars contributing significantly to the overall light.
