The galaxy appears as a generally smooth object, exhibiting a somewhat elliptical morphology. The central region presents a bright, concentrated luminosity, decreasing in intensity towards the outer edges. There is little to no evidence of prominent spiral arm structures or a well-defined disk. The galaxy's color profile is largely dominated by redder wavelengths, suggesting an older stellar population, though there may be some presence of bluer wavelengths. There appears to be some slight disruption to the shape of the galaxy suggesting minor disturbances within the galaxy's morphology. Overall, the galaxy appears to be an evolved system.
