The galaxy presents an elliptical morphology, appearing relatively smooth with a concentrated central bulge. The color profile suggests a relatively evolved stellar population, with redder hues dominating the core region. The galaxy exhibits a degree of elongation and an angle of inclination relative to our line of sight, which informs its shape. There is no evident disk structure or spiral arm features that can be discerned from this image. There may be a hint of minor disturbance in the morphology, possibly due to a past or ongoing interaction, but it is otherwise isolated.
