The galaxy presents as a primarily smooth, elliptical morphology. Its light distribution appears centrally concentrated, fading gradually towards the outer edges. There's a notable lack of distinct spiral arm structures or prominent dust lanes. The color profile suggests an older stellar population, characterized by a reddish-yellow hue. There is no evidence of on-going major merging activity, but subtle asymmetries or minor disturbances cannot be ruled out based on the current image resolution. The galaxy's overall appearance suggests a relatively evolved system, potentially with low levels of recent star formation.
