This galaxy exhibits a prominent disk structure, but without a clearly defined spiral arm morphology. The central bulge is significant and appears relatively smooth and featureless, displaying a yellowish-white color indicative of an older stellar population. The disk shows a bluer hue, implying the presence of younger, hotter stars and ongoing star formation. There is a suggestion of some structure within the disk, perhaps indicative of faint spiral arms or dust lanes, but the image resolution limits detailed assessment. The galaxy does not exhibit strong signs of tidal disruption or a major merger event, though a minor disturbance cannot be ruled out based on the faint irregularities observed. Overall, the galaxy appears to be a relatively evolved system undergoing moderate star formation activity.
