The galaxy appears as a moderately bright, relatively smooth object. It exhibits an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated. There may be a slight asymmetry or minor disturbance in its overall structure, potentially indicating a past or ongoing interaction with another galaxy. The light distribution is mostly uniform, lacking strong central concentration or distinct spiral arms. The color suggests a stellar population dominated by older stars, with low to moderate levels of ongoing star formation. The overall morphology suggests a galaxy that could be classified as an early-type spiral galaxy. The diameter spans approximately 3 kpc.
