The galaxy presents a generally smooth morphology, with a high degree of central concentration of light. It appears predominantly round, with a hint of ellipticity. The galaxy's color profile is relatively uniform, showing a moderate red-shift, possibly indicating an older stellar population and low ongoing star formation. There is no obvious evidence of strong spiral arm structure or prominent dust lanes. The absence of strong irregularities suggests that the galaxy is likely not undergoing a major merger or strong tidal interaction. There is a low chance it could be experiencing a minor merger.
