The galaxy presents as a somewhat smooth, elliptical-like morphology. The light is concentrated towards the center of the galaxy, which appears more luminous with a yellowish hue, suggesting an older stellar population and potentially a lower rate of ongoing star formation. The isophotes suggest a slight elongation, but overall it maintains a fairly circular appearance. A faint, small extension of light appears to be close to the main component of the galaxy; this feature could be a tidal tail or a companion galaxy that is merging. The galaxy does not show any prominent spiral arms or dust lanes.
