The galaxy presents as a somewhat elongated system, exhibiting a moderate degree of ellipticity. The central region shows a bright, concentrated bulge with a yellowish hue, suggesting an older stellar population. Fainter, bluer light extends outwards from the bulge along the major axis, indicating the presence of a disk component. There are indications of some internal structure within the disk, including hints of arm-like features and dust lanes, but their morphology is not well-defined. The system appears relatively smooth overall, with a lack of prominent spiral arms or intense star-forming regions. The galaxy's color suggests a mix of stellar populations, with the bulge dominated by older, redder stars, and the disk containing younger, bluer stars. There might be a low level of ongoing star formation, but no intense star formation events are readily apparent.
