The galaxy presents a somewhat elliptical morphology, appearing generally smooth and featureless in this image. A concentrated central bulge exhibits a yellowish-white hue, indicating a likely population of older stars. Extending outwards from the bulge, a fainter, bluer disk-like structure is discernible. The transition between the bulge and the disk appears relatively gradual. There is little evidence of spiral arm structure or prominent dust lanes within the disk. The overall appearance suggests a relatively evolved galaxy with a moderate level of ongoing star formation. The elongation indicates that the system is viewed at an angle. No clear signs of recent or ongoing major mergers are detected, though a minor interaction is not completely ruled out by the image alone.
