The galaxy appears as a centrally concentrated, elliptical-like system. The light distribution is relatively smooth, with no obvious spiral arm structures or prominent dust lanes visible at this resolution. The galaxy exhibits a somewhat rounded morphology. There are hints of a slight elongation in the light distribution, but this is minimal. A concentrated central bulge is apparent, surrounded by a more diffuse halo. The galaxy appears to be in a relatively quiescent state, with a low specific star formation rate. No major disturbances or signs of recent merger events are apparent.
