The galaxy presents a somewhat elliptical morphology, appearing as a lenticular-type galaxy. Its core exhibits a brighter, more concentrated luminosity which fades outward. The galaxy shows a smooth texture, suggesting an older stellar population. There is no visible evidence of spiral arms or prominent dust lanes. The color indices suggest it is generally redder than actively star-forming galaxies. No major mergers or significant tidal disturbances are readily apparent. There appears to be a slight elongation, though the overall shape is fairly regular. The galaxy's estimated physical size is around 5.7 kpc, indicating it is a dwarf galaxy.
