The galaxy presents as a roughly elliptical, smooth object. The light distribution appears centrally concentrated. The galaxy has a cyan hue. There is evidence of a faint outer envelope, suggesting possible past interactions or accretion events. No obvious spiral arm structures or dust lanes are visible, giving the galaxy a smooth appearance. The overall morphology indicates a spheroid-dominated system, with little evidence of recent star formation, the lack of redder color implies there is some star formation. The object exhibits a moderate degree of roundness. Evidence of disturbance suggests potential minor or major interactions or a possible recent merger.
