The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears fairly uniform, lacking distinct spiral arms or prominent dust lanes. There is a color gradient visible, with the central region exhibiting a yellowish hue, which suggests a population of older, redder stars. The outer regions show a subtle shift towards bluer colors, hinting at some ongoing or recent star formation, however subdued. The overall shape is close to round, with no major disturbances or signs of an ongoing merger readily apparent. The galaxy appears to be well-defined against the background, indicating a notable density contrast. The size is moderately compact, suggesting a dwarf or intermediate-sized galaxy.
