The galaxy presents an elliptical morphology, with a major axis roughly twice the length of its minor axis. The central region exhibits a high surface brightness, appearing nearly spherical and intensely luminous, suggesting a concentrated stellar population, likely older stars. The isophotes are elongated and appear boxy, with a slight tilt. The galaxy displays a smooth luminosity gradient, fading gradually from the core outwards. There is a hint of a diffuse, extended halo surrounding the main body of the galaxy, although the boundary is indistinct. The overall color appears somewhat redder than the surrounding field, which is consistent with an older stellar population and relatively low star formation activity. A low level of dust extinction may be present, contributing to the redder color. There are no prominent spiral arms or other features indicative of ongoing, major star formation.
