The galaxy presents as a relatively smooth, elliptical object, elongated slightly along one axis, suggesting it is likely a disk galaxy with some inclination. The central region exhibits a high surface brightness, indicating a concentrated core that may contain a supermassive black hole. Fainter, diffuse light extends outwards from the core, gradually fading into the background. The colour appears to be dominated by yellow and red wavelengths, suggestive of an older stellar population, with a small amount of recent star formation indicated by some bluer light. No distinct spiral arm structures or prominent dust lanes are discernible. There is a suggestion of minor gravitational disturbance within the galaxy.
