The galaxy presents as a relatively smooth, elliptical morphology. The light profile appears centrally concentrated, exhibiting a gradual decline in intensity from the core outwards. The dominant color is a warm yellowish hue, suggesting a stellar population dominated by older, redder stars. There are also some regions of green to blue color, indicating either the presence of younger populations of stars or perhaps some emission lines. There is no apparent spiral structure or prominent dust lanes. The galaxy appears fairly isolated. It is a relatively round shape, with no obvious major disturbances.
