The galaxy presents as a largely featureless elliptical or lenticular system. It exhibits a smooth, concentrated light profile, with a radial gradient indicating a dense central region. The color appears relatively uniform and red-yellow, suggesting an older stellar population. There is no discernible evidence of spiral arms or significant dust lanes. The overall morphology indicates a lack of ongoing star formation. The round shape suggests it is a relatively relaxed system, and does not show any evidence of a major merger. Slight irregularities may point to minor tidal disturbances.
