The galaxy presents as a relatively smooth, disk-like structure, possibly a spiral galaxy seen at an angle. The central bulge is a prominent, concentrated area of yellowish-white light, suggesting a dense population of older stars. Fainter spiral arms appear to emanate from the central bulge, though their structure is somewhat irregular and not sharply defined. One arm has a strong, yellowish light and the other is of a faint bluish-white color. There is a hint of disturbance to the disk, possibly indicative of a past or ongoing minor interaction or merger. The overall color suggests a mix of stellar populations, with the bulge dominated by older, redder stars and the arms potentially containing younger, bluer stars. The galaxy exhibits intermediate characteristics between a pure elliptical and a well-defined spiral galaxy.
