The galaxy presents as an intermediate spiral with a relatively smooth appearance. It is elongated, with a discernible bulge. The central region exhibits a yellowish hue, suggesting an older stellar population, indicative of lower star formation. Fainter, bluer regions are observed to one side of the galaxy, suggesting ongoing star formation, likely in a disk component. The overall structure is mildly disturbed, which suggests a possible interaction with a smaller object or past merger event. The disk appears to be slightly warped and irregular, rather than cleanly defined. There are no apparent signs of a strong tidal tail or a significant major merger. Overall, it appears to be an evolved spiral galaxy, exhibiting characteristics of both early- and late-type spirals.
