The galaxy presents as a moderately luminous, relatively smooth object. Its shape appears to be somewhere between elliptical and a disk galaxy; tending toward the elliptical end of the spectrum. A central bulge is prominent, exhibiting a yellowish to reddish hue, indicative of an older stellar population with lower star formation rates. The outer regions transition into a bluer color, implying younger stars and ongoing, but not vigorous, star formation. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy is not perfectly spherical; It shows some flattening. There is no clear evidence of major mergers or significant tidal disturbances in its immediate vicinity, although a faint irregularity in shape suggests potentially a past minor interaction or accretion event. The galaxy is unresolved and roughly 7 kpc across.
