The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light distribution. It appears largely spheroidal. The color profile suggests an older stellar population, with a noticeable red-yellow hue, indicative of evolved stars. There is no discernible spiral structure or prominent dust lanes visible. A slight asymmetry is observed, potentially resulting from a minor gravitational interaction with a faint object nearby, or from internal activity. The system appears relatively isolated, without signs of ongoing major merging events.
