The galaxy presents a generally smooth appearance, with a diffuse, elliptical morphology. A bright central bulge is observed, with light gradually decreasing outwards. The galaxy exhibits a blueish hue overall, suggesting the presence of some younger stellar populations, however, the low star formation rate indicates that it is not actively forming stars at a high rate.  The galaxy appears to be relatively isolated, without obvious signs of major interaction or merging with other galaxies, however, there is a possibility of minor disturbance in the structure. It is neither perfectly circular nor highly elongated, appearing more of an intermediate elliptical shape.
