The galaxy presents as a relatively smooth, elongated structure with a discernible central bulge. The light distribution suggests a Sersic profile, concentrated towards the core. The galaxy exhibits a noticeable color gradient, transitioning from a bluer hue in the outer regions to a yellower/whiter hue closer to the nucleus, potentially indicating a change in stellar population or dust content towards the galactic center. The ellipticity is significant, implying a flattened, disk-like morphology viewed at an angle. No prominent spiral arms or bar structures are immediately apparent in the image. The galaxy does not appear to be undergoing any major merging events, although there may be a slight disturbance or asymmetry in the outer halo. The overall appearance suggests a relatively evolved system.
