This galaxy exhibits a morphology that is predominantly smooth, with a slight suggestion of disklike structure. The central region is noticeably brighter and has a yellowish hue, potentially indicating a higher concentration of older stellar populations. Moving outward from the center, the galaxy gradually fades in intensity, with subtle hints of bluer colors in the outer regions, implying the presence of some younger stars. The overall shape of the galaxy appears somewhat elongated, but generally lacks any substantial distortions or tidal features indicative of major interactions. There are faint, diffuse features or arms visible in the outskirts, which are slightly disturbed. The galaxy seems to be in a relatively isolated state, showing no signs of an ongoing major merger.
