This galaxy presents as a relatively bright, though somewhat compact, system. The central region exhibits a concentrated, yellowish hue, suggesting a population of older stars. Moving outward from the core, the disk of the galaxy is apparent, showing a bluer color profile, indicative of more recent star formation, with hints of redder regions in the disk. The overall morphology appears intermediate between elliptical and spiral. The disk does not exhibit well-defined spiral arms but rather shows subtle, irregular features, suggesting either a disturbed morphology or a flocculent spiral structure. The galaxy appears to be undergoing a period of intermediate star formation activity, as evidenced by both the older stellar population in the core and the presence of younger, bluer stars in the disk. There is potential evidence of interaction or merging history due to subtle distortions in the outer regions of the disk.
