The galaxy presents as a spiral type, observed at a slight inclination. The central bulge is moderately prominent, appearing bright white, indicative of an older stellar population. Faint spiral arms appear to emerge from the central region and extend outwards. These arms exhibit a bluer hue, suggesting ongoing star formation, though this is subdued compared to the bulge. There may be a faint bar structure within the central region. Overall, the galaxy has a relatively smooth appearance, with a suggestion of a disturbed morphology, but does not appear to be actively merging.
